May 01 - 03, 2002
NASA-Ames Research Center, Moffett Field, California
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AUTHORS
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TITLES
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Mian M. ABBAS, Paul D. Craven, James F. Spann, et al.; (NASA Marshall Space Flight Center, Huntsville, Alabama); Dragana Tankosic; (University of Alabama at Huntsville, Huntsville, Alabama) |
Laboratory studies of the optical properties and condensation processes of cosmic dust particles |
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L. J. ALLAMANDOLA; (Astrochemistry Laboratory, NASA Ames Research Center) |
Infrared emission from interstellar PAHs, new probes of the interstellar medium |
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Aldo J. APPONI, Lucy M. Ziurys, Philip M. Sheridan, Matthew A. Brewster, Chandra Savage; The University of Arizona, Depts Chemisty and Astronomy, 933 N. Cherry Ave., Tucson, AZ 85721 |
Submillimeter spectroscopy of astrophysically important metal-containing molecules |
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J.F. BABB and K. Kirby; Harvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA 02138; H.-K. Chung; Lawrence Livermore National Laboratory, Livermore, CA, 94550 |
Theoretical studies of pressure broadened alkali-metal atom resonance lines |
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E.L.O. BAKES, Hiroshi Imanaka, S. Lebonnois, C.W. Bauschlicher and C.P. McKay |
The role of laboratory investigations in elucidating the nature of organic molecules in the titan haze |
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E.L.O. BAKES, C.W. Bauschlicher, and A.G.G.M. Tielens |
A state of the art infrared spectral analysis of the chemical evolution of carbonaceous molecules during star formation |
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Ehud BEHAR, Steven M. Kahn, Frits Paerels; Columbia University |
Observations of inner-shell soft X-ray absorption |
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P. BEIERSDORFER, H. Chen, M. May, D. Thorn; Lawrence Livermore National Laboratory; K. R. Boyce, G. V. Brown, R. L. Kelley, F. S. Porter, C. K. Stahle, A. Szymkowiak; NASA Goddard Space Flight Center; S. M. Kahn; Columbia University |
Laboratory studies of the X-ray emission generated by the interaction of solar wind heavy ions with comets |
| Edwin BERGIN; Harvard-Smithsonian Center for Astrophysics | Missing pieces in our understanding of astrochemistry: The answers are in the lab [invited talk] |
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L. BIENNIER, F. Salama, L. J. Allamandola; NASA Ames Research Center, Space Science Division, Moffett Field, CA 94035, USA; J. J. Scherer, A. O'Keefe; Los Gatos Research, 67 East Evelyn Ave., Suite 3, Mountain View, CA 94041, USA |
Gas phase spectroscopy of cold PAH ions: Contribution to the interstellar extinction and the diffuse interstellar bands |
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W. J. BORUCKI and David G. Koch; (NASA Ames Research Center),; Gibor Basri; (Univ. Calif., Berkeley, CA),; William Cochran; (Univ. Tex., Austin, TX),; Edward W. Dunham; (Lowell Observatory, Flagstaff, AZ); Ronald Gilliland; (STScI, Balitmore, MD); Jon M. |
Stellar and planetary data products expected from the Kepler mission |
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G. V. BROWN {Currently supported by an NRC research associateship}, K. R. Boyce, R. L. Kelley, F. S. Porter, C. K. Stahle, A.E. Szymkowiak, and W. Tillotson; NASA Goddard Space Flight Center; P. Beiersdorfer, H. Chen, M. J. May, and D. Thorn; Lawrence Liv |
Laboratory astrophysics at the LLNL electron beam ion traps EBIT-I & EBIT-II |
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G. V. BROWN; NASA Goddard Space Flight Center, Greenbelt, MD; P. Beiersdorfer, H. Chen, M. H. Chen, and K. J. Reed; Lawrence Livermore National Laboratory |
Laboratory study of the diagnostic utility of the 3C/3D line ratio in Fe XVII |
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L. R. BROWN; (Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA); and M. Dulick; (National Solar Observatory, Tucson, AZ) |
Empirical line intensities of methane in the near-infrared |
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G.M. Muñoz CARO, 1; U.J. Meierhenrich,2; W.A. Schutte,1 B. Barbier2, A. Arcones Segovia,1; H. Rosenbauer,3 W.H.-P. Thiemann,4 A. Brack,2 J.M. Greenberg1; (1. Raymond and Beverly Sackler Laboratory for Astrophysics at Leide, The Netherlands); (2. Centre d |
Formation of chiral organic molecules in simulated dense cloud environments |
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Pisin CHEN; Stanford Linear Accelerator Center, Stanford University, Stanford, CA 94309 |
A facility for laboratory astrophysics using high intensity particle and photon beams |
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A. CHUTJIAN, Steven J. Smith, and J. A. Lozano; Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA USA |
Measurement of absolute excitation cross sections in highly-charged ions using electron energy loss and merged beams |
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A. CHUTJIAN, I. Cadez, J. B. Greenwood, R. J. Mawhorter, and S. J. Smith; Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA USA |
Laboratory measurements of solar-wind/comet X-ray emission and charge-exchange cross sections |
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Geoffrey C. CLAYTON, L. Valencic; Lousiana State University; K. D. Gordon; Steward Observatory; M.J. Wolff; SSI |
Unification: UV & IR observations of interstellar dust along the same sightlines |
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R. J. CODY W. A. Payne, R. P. Thorne, Jr., P. N. Romani, L. J. Stief (NASA/Goddard Space Flight Center), F. L. Nesbitt (Coppin State College), M. A. Iannone (Millersville University), D. C. Tardy (University of Iowa) |
Temperature dependence of the rate constant for the CH3 recombination reaction: a loss process in outer planet atmospheres |
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Mark P. COLLINGS, Helen Fraser, John W. Dever and Martin R.S.McCoustra; (School of Chemistry, University of Nottingham, UK) |
Laboratory surface science: The key to the gas-grain interaction |
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David M. CORNELISON and T.R. Dillingham; Northern Arizona University |
Color changes in ices due to irradiation by ultraviolet and X-ray photons |
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P. C. COSBY, D. L. Huestis, and J. R. Peterson; (Molecular Physics Laboratory, SRI International) |
Experimental measurements of dissociative recombination relevant to planetary atmospheres |
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Dale P. CRUIKSHANK; (NASA Ames Research Center) |
A solar system perspective on laboratory astrophysics [invited talk] |
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J. B. DALTON; NASA-Ames Research Center |
Cryogenic reflectance spectra in support of planetary missions |
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Louis B. D’HENDECOURT; (Institut d'Astrophysique Spatiale, "Astrochimie Expérimentale,"; Campus d'Orsay, ORSAY, FRANCE) |
The PAH hypothesis: A dream or a nightmare for astrophysicists? [invited talk] |
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B. J. DROUIN, J.C. Pearson, H. M. Pickett and P. Chen; Jet Propulsion Laboratory, California Institute of Technology, Mail Stop 183-301, Pasadena, CA 91109 |
Microwave, millimeter, submillimeter and far infrared spectroscopy at the Jet Propulsion Laboratory |
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Jason P. DWORKIN*, Scott A. Sandford, Max P. Bernstein*, and Louis J.Allamandola; NASA-Ames Research Center, MS 245-6, Moffett Field, CA 94035 USA; *Also of the Center for the Study of Life in the Universe, SETI Institute, 2035 Landings Drive, Mountain Vi |
The laboratory production of complex organic molecules in simulated interstellar ices |
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Brian EICHELBERGER, Theodore Snow*, Cynthia Barckholtz, Momir Stepanovic,; and Veronica Bierbaum; (University of Colorado at Boulder, Department of Chemistry and Biochemistry); (*University of Colorado at Boulder, Center for Astrophysics and Space Astrono |
Laboratory anion chemistry: implications for the dibs, and a potential formation mechanism for a known interstellar neutral molecule |
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M. Samy EL-SHALL and Michael Meot-Ner; Department of Chemistry, Virginia Commonwealth University, Richmond, VA 23284-2006 |
Organic chemistry and nanoparticles in astrophysics |
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Gary J. FERLAND; (Dept. of Physics, University of Kentucky) |
Laboratory astrophysics' needs for understanding photoionized plasmas |
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George J. FLYNN; (Dept. of Physics, SUNY-Plattsburgh, Plattsburgh, NY) |
Synchrotron FTIR examination of interplanetary dust particles: An effort to determine the compounds and minerals in interstellar and circumstellar dust |
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H. J. FRASER, E. F. van Dishoeck; Raymond and Beverly Sackler Laboratory for Astrophysics, Leiden Unviersity, Postbus 9513, 2300RA, Leiden, Netherlands; X. Tielens; Kapteyn Institute, Rijksuniversiteit Groningen, Postbus 800, 9700AV, Groningen; Netherland |
Deciphering chemical reactions in icy environments |
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Friedemann FREUND (1), Minoru Freund (2), Aaron Staple (3), and John Scoville(4); 1. SETI Institute/SJSU/NASA Ames; 2. NASA GSFC; 3. Stanford University; 4. University of Kentucky |
Nature of the organic signature in dust from the interstellar medium: laboratory analog studies |
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Friedemann T. FREUND (1), John Scoville (2), Reimer Holm (3), Rudolf Seelemann3,; and Minoru M. Freund (2); 1. SETI Institute/SJSU/NASA Ames; 2. University of Kentucky; 3. BAYER AG (Leverkusen, Germany); 4. NASA GSFC |
C-H hot bands in the near-IR emission spectra of leonids |
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Perry A. GERAKINES and Thomas J. Wdowiak; Astro- and Solar-System Physics Program, Department of Physics, University of Alabama at Birmingham, 1300 University Blvd, CH310, Birmingham, AL 35294-1170 |
Maldi-TOF MS technology considerations relevant to an exobiology surface-science approach for Europa |
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Thomas F. GIESEN; (Physikalisches Institut, Universitaet zu Koeln, Germany) |
Laboratory spectroscopy of interstellar molecules |
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A.E. GLASSGOLD; (New York University and University of California, Berkeley) |
Microscopic processes in X-ray modulated star formation |
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T. W. GORCZYCA and O. Zatsarinny; Department of Physics, Western Michigan University, Kalamazoo, MI 49008 |
Computation of dielectronic recombination data for the oxygen-like isoelectronic sequence |
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T. W. GORCZYCA; Department of Physics, Western Michigan University,; Kalamazoo, MI 49008; N. R. Badnell; Department of Physics and Applied Physics, University of Strathclyde, Glasgow, G4 0NG, UK; D. W. Savin; Columbia Astrophysics Laboratory, Columbia Uni |
Shortcomings of the R-matrix method for treating dielectronic recombination |
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Carl A. GOTTLIEB, Philip C. Myers, Edwin A. Bergin, and Patrick Thaddeus; Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138; Mario Tafalla; Observatorio Astronomico Nacional, Alfonso XII, 3, E-28014 Madrid, Spain |
Precise laboratory measurements of line frequencies useful to studies of star and planet formation |
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James GREEN (Center for Astrophysics and Space Astronomy, University of Colorado at Boulder) |
The cosmic origins spectrograph |
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Tom GREENE (NASA Ames Research Center) |
The Sofia mission and laboratory astrophysics synergies |
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U. GRIESMANN and W. L. Wiese: National Institute of Standards and Technology, Gaithersburg, MD 20899 |
Atomic oscillator strengths by emission spectroscopy and lifetime measurements |
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Murthy S. GUDIPATI (1,3) Richard A. Copeland (2), Marshall L. Ginter (1); (1) Institute of Physical Sciences and Technology, University of Maryland, College Park, MD 20742; (2) Molecular Physics Laboratory, SRI International, 333 Ravenswood Avenue, Menlo |
Temperature dependent collisional energy transfer of N2 (A, V = 0 and 1): The upper state of LBH-emission |
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Murthy S. GUDIPATI; Institute of Physical Sciences and Technology, University of Maryland,} College Park, MD 20742; and; Visiting Scientist at Molecular Physics Laboratory, SRI International, 333 Ravenswood Avenue, Menlo Park, CA; 94025 |
Near-infrared emission of highly excited CO - A more sensitive method to probe the interstellar matter?? |
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Martin HARWIT, Emeritus Professor of Astronomy, Cornell University |
Current and future space missions. Great questions of the next decade in connection with laboratory astrophysics [introductory talk] |
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C. C. HAVENER, C. R. Vane, and H. F. Krause; Oak Ridge National Laboratory, Physics Division, P.O. Box 2008, MS 6372 Oak Ridge, TN 37831-6372; D. W. Savin; Columbia Astrophysics Laboratory, Columbia University, New York, NY 10027 |
Laboratory measurements of charge transfer on atomic hydrogen at thermal energies |
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Martin HEAD-GORDON (1), Jennifer L. Weisman (1), and Timothy J. Lee (2); 1) Department of Chemistry, University of California, Berkeley, CA 94720, and,; 2) NASA Ames Research Center, Moffett Field, CA 94035 |
Electronic structure calculations on excited states of polycyclic aromatic hydrocarbon ions |
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R. F. HEETER, M. E. Foord, D. A. Liedahl, and P. T. Springer; Lawrence Livermore National Laboratory, L-043; P.O.Box 808; Livermore, CA 94551; J. E. Bailey and M. E. Cuneo; Sandia National Laboratories, Albuquerque; F. Keenan, M. Phillips and P. van Hoof; |
Benchmarking accretion disk models using photoionized laboratory plasmas |
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Thomas HENNING; Astrophysical Institute and University Observatory (AIU), Schillergasschen 3, D-07745 Jena, Germany; and Max Planck Institute for Astronomy, Konigstuhl 17, D-69117 Heidelberg, Germany |
Nanoparticles in space and the laboratory [invited talk] |
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E. HERBST, F. C. De Lucia, R. A. H. Butler, M. Winnewisser; Department of Physics, The Ohio State University, Columbus, OH 43221 |
The submillimeter-wave spectra of interstellar molecules |
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David L. HUESTIS; Molecular Physics Laboratory, SRI International, Menlo Park, CA 94025; Jeffery A. Spirko and A. Peet Hickman; Department of Physics, Lehigh University, Bethlehem, PA 18015 |
Charge transfer collisions in ionospheres, exospheres, and interstellar clouds |
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Hantao JI, Masaaki Yamada, and Russell Kulsrud; Princeton Plasma Physics Laboratory, Princeton University |
Laboratory study of physics of magnetic reconnection |
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William E. JOHNSTON, Tom Hinke, Tony Lissota, Piyush Mehrotra, and Arsi Vaziri; (Lawrence Berkeley National Laboratory) |
Computing and data grids: infrastructure for large-scale collaborative science |
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M. JURA; UCLA |
SIRTF: Goals and requirements |
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Steven M. KAHN; Columbia University |
High energy astrophysics - X-ray spectroscopy and atomic data [invited talk] |
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K. S. KALOGERAKIS G. Amaral, T. G. Slanger P. C. Cosby, D. L. Huestis, and R. A. Copeland; Molecular Physics Laboratory, SRI International, Menlo Park, CA 94025 |
Research on electronically- and vibrationally-excited O2, with application to planetary and terrestrial atmospheres |
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Kate KIRBY |
Report Talk: ICAMDATA & APiP |
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Victor H.S. KWONG, De Chen, and H. Gao; Department of Physics, UNLV, 4505 Maryland Parkway, Las Vegas, NV 89154 |
Charge transfer between S2+ and H2 at electron volt energies |
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J. Martin LAMING; Space Science Division, US Naval Research Laboratory, Washington DC 20375; Jacob Grun, C. Moore, T. Jones; Plasma Physics Division, US Naval Research Laboratory, Washington DC 20375; C. Manka; Research Support Instruments; D. Tam; Naval |
Radiative shock instabilities from the laboratory to Cassiopeia A |
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J. E. LAWLER and E. A. Den Hartog,; (Dept. of Physics, Univ. of Wisconsin, Madison); C. Sneden; (Dept. of Astronomy and McDonald Observatory, Univ. of Texas, Austin) |
Improved radiative lifetimes, branching fractions and atomic transition probabilities for Nd II |
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J. K. LEPSON; University of Califonia, Berkeley; P. Beiersdorfer, H. Chen, D. Thorn; Lawrence Livermore National Laboratory; E. Behar, S. M. Kahn; Columbia University |
Spectral catalogue of intermediate charge states of high-Z ions for astrophysical diagnostics in the euv and soft X-ray |
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Steven T. MANSON; Georgia State University; Himadri S. Chakraborty; Kansas State University; Pranawa C. Deshmukh; Indian Institute of Technology-Madras |
Interchannel coupling in the photoionization of ions |
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A.L. MATTIODA, D.M. Hudgins, C.W. Bauschlicher, Jr., and L.J. Allamandola; (NASA Ames Research Center) |
Infrared spectroscopy of matrix-isolated polycyclic aromatic hydrocarbons and associated ions. PAHs incorporating pyrene and peropyrene structures |
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A.L. MATTIODA, D.M. Hudgins, C.W. Bauschlicher and L.J. Allamandola; (NASA Ames Research Center) |
Infrared spectra of matrix-isolated heterocyclic aromatic compounds and their ions |
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B. J. MCCALL; Department of Astronomy & Department of Chemistry, University of California; at Berkeley; B. L. Rachford, T. P. Snow; Center for Astrophysics and Space Astronomy, University of Colorado at Boulder; P. Sonnentrucker, S. Friedman; Department o |
Early results from the APO diffuse interstellar band survey |
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M.H. MOORE; (NASA Goddard Space Flight Center); R.L. Hudson; (Eckerd College and NASA Goddard Space Flight Center); R.F. Ferrante; (US Naval Academy and NASA Goddard Space Flight Center) |
Synthesis of HCN and HNC in ion-irradiated N2-rich ices |
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Cheuk-Yiu NG; (Department of Chemistry, University of California, Davis) |
Determination of accurate energetic database for combustion, atmospheric, and interstellar chemistry |
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Joseph A NUTH III1, Frans J. M. Rietmeijer2 and Hugh G. M. Hill3; (1. Astrochemistry Branch, NASA's Goddard Space Flight Center); (2. Inst. of Meteoritics, Dept. Earth & Planetary Sciences, Univ. New Mexico, Albuquerque); (3. NAS/NRC Resident Research Ass |
Condensation processes in astrophysical environments: The composition and structure of cometary grains |
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J. C. PEARSON; (Jet Propulsion Laboratory, California Institute of Technology) |
High-resolution photoionization and photoelectron studies: Laboratory astrophysics needs of the Herschel Space Observatory |
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J.C. PEARSON, H. M. Pickett, B. J. Drouin, P. Chin, and E. A. Cohen; (Jet Propulsion Laboratory, California Institute of Technology) |
Microwave, millimeter, submillimeter and far infrared spectral databases |
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Y. PENDLETON and Lou Allamandola (NASA Ames Research Center) |
The organic refractory material in the diffuse interstellar medium: Mid-IR spectroscopic constraints |
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Ruth C. PETERSON; Astrophysical Advances and UCO/Lick |
Empirical near-UV line parameters from hubble spectroscopy |
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Juliet C. PICKERING Anne P. Thorne and Richard Blackwell-Whitehead; Blackett Laboratory, Imperial College, London SW7 2BZ, UK |
Laboratory astrophysics and high resolution atomic spectroscopy with the Imperial College fourier transform spectrometer |
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PIZAGNO, J. and Sellgren, K. (Department of Astronomy, The Ohio State University); Uchida, K. I. (RS Science Center, Center for Radiophysics Space Research, Cornell University); Werner, M. W. (Jet Propulsion Laboratory) |
The energetics of the 12 micron IRAS band |
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F. S. PORTER, K. R. Boyce, G. V. Brown, R. L. Kelley, C. K. Stahle, and W. Tillotson; NASA/Goddard Space Flight Center, Greenbelt, Maryland; P. Beiersdorfer, H. Chen, M. May, and D. Thorn; Lawrence Livermore National Laboratory, Livermore, California; S. |
Laboratory astrophysics with a high-resolution XRS X-ray microcalorimeter |
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J. READER, W. L. Wiese, W. C. Martin, A. Musgrove, and J. R. Fuhr; National Institute of Standards and Technology, Gaithersburg, MD 20899, U.S.A. |
NIST databases on atomic spectra |
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T.L. ROUSH 1 and J.B. Dalton1,2; 1. NASA Ames Research Center; 2. NRC, Resident Research Associate |
Cryogenic Titan tholins |
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Richard RUITERKAMP; Leiden Observatory, P.O. Box 9513, 2300 RA Leiden, The Netherlands; Thomas Halasinski, Farid Salama; NASA-Ames Research Center, Space Science Division, Moffett Field, CA 94035-1000,; USA; Bernard Foing; ESA Space Science, ESTEC/SCI-SR |
Laboratory calibration studies in support of an ISS exposure experiment and comparison to the diffuse interstellar bands |
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Scott A. SANDFORD; NASA-Ames Research Center, MS 245-6, Moffett Field, CA 94035 USA |
The Astrobiology Explorer (ABE) midex mission concept: using infrared spectroscopy to identify organic molecules in space |
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D. W. SAVIN; Columbia Astrophysics Laboratory, Columbia University, New York, NY 10027; G. Gwinner, D. Schwalm, and A. Wolf; Max-Planck Institut fur Kernphysik, Heidelberg, Germany; A. Muller and S. Schippers; Institut fur Kernphysik, Strahlenzentrum der |
Ion storage ring measurements of low temperature dielectronic recombination rate coefficients for modeling X-ray photoionized cosmic plasmas |
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Daniel Wolf SAVIN; Columbia Astrophysics Laboratory, Columbia University, New York, NY 10027 |
Rate coefficients For D(1s) + H^+ <--> D^+ + H (1s) charge transfer and some astrophysical implications |
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Richard J. SAYKALLY; Department of Chemistry, University of California, Berkeley, CA 94720-1460 USA |
Molecular carbon in the galaxy: New laboratory and observational studies |
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Brian SHARPEE, Jack Baldwin; Michigan State University; Robert Williams; Space Telescope Science Institute; Peter van Hoof; Queen's University Belfast |
EMILI - An aid in emission line identification in emission-line regions |
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T. G. SLANGER, P. C. Cosby, and D. L. Huestis; Molecular Physics Laboratory, SRI International, Menlo Park, CA |
The atmosphere as laboratory: Aeronomy by astronomy |
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Gregory P. SMITH and David L. Huestis; Molecular Physics Laboratory, SRI International, Menlo Park, CA |
Low-temperature hydrocarbon photochemistry: CH3 + CH3 recombination in giant planet atmospheres |
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Peter L. SMITH; Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138; Juliet C. Pickering and Anne P. Thorne; Blackett Laboratory, Imperial College, London SW7 2BZ, UK |
New atomic data for doubly ionized 3d transition group elements by high resolution fourier transform spectroscopy |
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Peter L. SMITH, J. Rufus, K. Yoshino, and W. H. Parkinson; Harvard-Smithsonian Center for Astrophysics; Glenn Stark; Physics Department, Wellesley College; J. C. Pickering and A. P. Thorne; Blackett Laboratory, Imperial College, London |
UV photoabsorption cross sections of CO, N2, AND SO2 [1mm] for studies of the ISM and planetary atmospheres |
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Steven J. SMITH and A. Chutjian; Jet Propulsion Laboratory, California Institute of Technology, Pasadena CA 91109 USA |
Measurements of lifetimes and F-values in highly-charged positive ions |
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T.L. SMITH, G.C. Clayton; Louisiana State University; K.D. Gordon, C. Engelbracht; Steward Observatory |
The newly discovered NIR features in NGC 7023 and other reflection nebulae |
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Christopher SNEDEN; Department of Astronomy McDonald Observatory, University of Texas at Austin; James E. Lawler; Department of Physics, University of Wisconsin at Madison; John J. Cowan; Department of Physics and Astronomy, University of Oklahoma; Harrie |
Atomic data and stellar chemical compositions [invited talk] |
| Ted SNOW, CASA Univ of Colorado | Report Talk: HST Science Legacy |
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P. C. STANCIL and J. G. Wang; Department of Physics and Astronomy and Center for Simulational Physics; D. R. Schultz and M. J. Rakovic; Physics Division, Oak Ridge National Laboratory; B. Zygelman; Department of Physics, University of Nevada, Las Vegas |
Charge transfer calculations and database for astrophysics |
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Hiroshi SUTO (Subaru Telescope, JAPAN), Takeshi Fukui, Satoshi Ohara (Japan Fine Ceramic Center, JAPAN), and Chiyoe Koike(Kyoto Pharmaceutical University, JAPAN) |
Fine particle production by spray pyrolysis method |
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Jan SZCZEPANSKI John Banisaukas, So Hirata, and Martin Vala; (Department of Chemistry and Center for Chemical Physics, University of Florida, Gainesville, FL) |
Pre-resonance raman spectrum of the C13H9 fluorene-like radical |
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E. TAKACS; MIT, 77 Mass Ave, 26-239, Cambridge MA 02139-4307; and University of Debrecen, Debrecen, Bem ter 18/A, H-4026, Hungary.; J. M. Laming; US Naval Research Laboratory, Code 7674L, Washington DC 20375; J. D. Gillapsy, J. V. Porto, I. Kink; National |
Spectroscopy of trapped ions with a microcalorimeter on the NIST electron beam ion trap |
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Margaret TOLBERT, Melissa Trainer, Dan Curtis and Owen Toon; (University of Colorado); and Chris McKay; (NASA Ames Research Center); and Doug Worsnop; (Aerodyne Research, Inc.) |
Laboratory studies of early Earth tholin particles |
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Gianfranco VIDALI, J.E.Roser; Syracuse University, Syracuse, N.Y.13244; G.Manico', V.Pirronello; Universita' di Catania, Catania, Italy |
Investigations of formation of molecular hydrogen on dust grain analogues |
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P. F. WECK, P. C. Stancil A. Schweitzer, and P. H. Hauschildt; Department of Physics and Astronomy and Center for Simulational Physics, The University of Georgia; K. Kirby; Harvard-Smithsonian Center for Astrophysics; Y. Yamaguchi and W. Allen; Center for |
Molecular line and continuum opacities for modeling of extrasolar giant planet and cool stellar atmospheres |
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L. M. WIESE G. A. Bonvallet, and J. E. Lawler (Dept. of Physics, Univ. of Wisconsin, Madison) |
Laboratory measurement of a Fe II fuse band oscillator strength |
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E.H. WISHNOW; (Lawrence Livermore National Laboratory); H.P. Gush, H. Halpern, and I. Ozier; (University of British Columbia) |
Submillimeter spectra of low temperature gases and gas mixtures |
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J. P. WRUBEL, N. I. Agladze, and A. J. Sievers; LASSP, Cornell University, Ithaca, NY 14853 |
Impurity-induced mm-wave absorption in amorphous ice |