Literature DB >> 11539184

Detection of the 2165 inverse centimeter (4.619 micron) XCN band in the spectrum of L1551 IRS 5.

S C Tegler1, D A Weintraub, L J Allamandola, S A Sandford, T W Rettig, H Campins.   

Abstract

We report the detection of a broad absorption band at 2165 cm-1 (4.619 microns) in the spectrum of L1551 IRS 5. New laboratory results over the 2200-2100 cm-1 wavenumber interval (4.55-4.76 microns), performed with realistic interstellar ice analogs, suggest that this feature is due to a CN-containing compound. We will refer to this compound as XCN. We also confirm the presence of frozen CO (both in nonpolar and polar matrices) through absorption bands at 2140 cm-1 (4.67 microns) and 2135 cm-1 (4.68 microns). The relative abundance of solid-state CO to frozen H2O is approximately 0.13 while the abundance of XCN seems comparable to that of frozen CO.

Entities:  

Keywords:  NASA Center ARC; NASA Discipline Exobiology; NASA Discipline Number 52-10; NASA Program Exobiology

Mesh:

Substances:

Year:  1993        PMID: 11539184     DOI: 10.1086/172825

Source DB:  PubMed          Journal:  Astrophys J        ISSN: 0004-637X            Impact factor:   5.874


  2 in total

1.  Self-assembling amphiphilic molecules: Synthesis in simulated interstellar/precometary ices.

Authors:  J Dworkin; D Deamer; S Sandford; L Allamandola
Journal:  Proc Natl Acad Sci U S A       Date:  2001-01-30       Impact factor: 11.205

Review 2.  The nature and evolution of interstellar ices.

Authors:  J E Chiar
Journal:  Orig Life Evol Biosph       Date:  1997-06       Impact factor: 1.950

  2 in total

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