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  1. No Access

    Chapter

    ISO-SWS Observations of Weak Bands of Trace Components of Ices Towards the Young Stellar Object W 33A

    ISO-SWS observations of the highly obscured young stellar object W 33A reveal two broad absorption features centered at 7.24 and 7.40 µm. The position and width of these features indicates that they are due to...

    W. A. Schutte, J. M. Greenberg, E. F. van Dishoeck in Astrophysics and Space Science (1998)

  2. No Access

    Article

    ISO-SWS Observations of Weak Bands of Trace Components of Ices Towards the Young Stellar Object W 33A

    ISO-SWS observations of the highly obscured young stellar object W 33A reveal two broad absorption features centered at 7.24 and 7.40 µm. The position and width of these features indicates that they are due to...

    W.A. Schutte, J.M. Greenberg, E.F. Van Dishoeck in Astrophysics and Space Science (1997)

  3. Article

    Homochirality as the signature of extra-terrestrial life

    A. J. MacDermott, L. D. Barron, A. Brack in Origins of life and evolution of the biosp… (1996)

  4. No Access

    Chapter and Conference Paper

    Each Chairperson Reflects on Their Session...

    Editorial comment: Some of the Chairpersons have provided us with a summary of the papers presented in their session, while others have given a summary of the discussion following the papers. We trust that reader...

    D. L. Block, J. M. Greenberg in New Extragalactic Perspectives in the New South Africa (1996)

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    Chapter and Conference Paper

    Formaldehyde and Methanol Dominated Ices Toward GL 2136

    Infrared spectroscopy towards the embedded massive protostellar object GL 2136 reveals 2 absorption features at 3.47 and 3.54 µm. Through comparison with spectra of laboratory ice mixtures, an identification with...

    W. A. Schutte, P. A. Gerakines, T. R. Geballe in The Role of Dust in the Formation of Stars (1996)

  6. No Access

    Book

  7. Article

    Comet Halley as an aggregate of interstellar dust and further evidence for the photochemical formation of organics in the interstellar medium

    Photolysis of mixtures of CO:NH3:H2O at 12 K results in the formation of an organic residue which is not volatile in high vacuum at room temperature. Analysis of this fraction by GC-MS resulted in the detection o...

    R. Briggs, G. Ertem, J. P. Ferris in Origins of life and evolution of the biosp… (1992)

  8. No Access

    Chapter and Conference Paper

    On the Possible Detection of Solid O2 in Interstellar Grains

    In various models of the chemistry of interstellar grains, solid O2 is formed by accretion as well as by surface reactions. In dense molecular cloud models, at a later stage of evolution of an interstellar grain,...

    P. Ehrenfreund, R. Breukers, L. d’Hendecourt in Astrochemistry of Cosmic Phenomena (1992)

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    Book

  10. No Access

    Chapter

    Astromacromolecules: Formation of Very Large Molecules in Interstellar Space

    The study of the physical and chemical processes taking place in the interstellar medium is made possible by the creation of laboratory conditions which simulate those relevant in space - low temperature, ultr...

    C. X. Mendoza-Gomez, J. M. Greenberg, G. B. Eijkel, J. J. Boon in Chemistry in Space (1991)

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    Chapter

    From Interstellar Dust to Comets to Comet Dust: A Test of the Interstellar Dust Model of Comets

    The interstellar dust model of comets is used as a basis to simultaneously satisfy various observational constraints and to derive the porosity of comet dust. The observational constraints are: (1) the strengt...

    J. M. Greenberg, J. I. Hage in Chemistry in Space (1991)

  12. Article

    Photochemical reactions on interstellar grains

    James P. Ferris, P. J. McCain in Origins of life and evolution of the biosp… (1989)

  13. No Access

    Chapter

    Bioastronomy — Search for Extraterrestrial Life

    The past three years have seen not only a growth in the activities of our commission, but an extension of its activities into important areas which have heretofore motivated too little activity. Of particular ...

    Frank D. Drake, George Marx, M. D. Papagiannis, R. D. Brown in Reports on Astronomy (1988)

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    Chapter and Conference Paper

    Molecular Diffusions in Ices — Implications for the Composition of Interstellar Grain Mantles and Comet Nuclei

    It is known that the ice composition of interstellar grains varies from one molecular cloud to another. These differences already start with different cloud formation conditions, such as temperature, gas phase...

    B. Schmitt, R. J. A. Grim, J. M. Greenberg in Experiments on Cosmic Dust Analogues (1988)

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    Chapter and Conference Paper

    Interstellar Circular Polarization and the Dielectric Nature

    Measurements of interstellar circular polarization are regarded as one of the essential constraints on theoretical models of interstellar grains. Observations accumulated since 1972 indicate that in all lines ...

    G. Chlewicki, J. M. Greenberg in Experiments on Cosmic Dust Analogues (1988)

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    Chapter

    Molecular Origin of the 216 NM Interstellar Hump

    Vacuum ultraviolet photochemical experiments have been performed in an argon matrix, at low temperature (− 12 K). It appears that starting from a variety of simple organic molecules photo-products are formed w...

    G. P. van der Zwet, M. S. de Groot, F. Baas in Polycyclic Aromatic Hydrocarbons and Astro… (1987)

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    Article

    Introduction

    J. M. Greenberg in Astrophysics and Space Science (1986)

  18. No Access

    Article

    The role of grains in molecular chemical evolution

    The observations of dust gas in diffuse and molecular clouds are shown to reflect not only their current state but their past history. The interpretation of infrared spectra of dust in molecular clouds using a...

    J. M. Greenberg in Astrophysics and Space Science (1986)

  19. Article

    Exobiological experiments on the first EURECA mission

    G. Horneck, J. Barrett, A. Bieger, H. Bücker in Origins of life and evolution of the biosp… (1986)

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    Chapter and Conference Paper

    Introduction

    I am honored to be asked to introduce this second ‘Jena’ meeting on interstellar dust at Georgenthal and I thank the organizers for making this possible. For some of us, interstellar dust had not only provided...

    J. M. Greenberg in The Role of Dust in Dense Regions of Interstellar Matter (1986)

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