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Detection of the 2165 inverse centimeter (4.619 micron) XCN band in the spectrum of L1551 IRS 5We report the detection of a broad absorption band at 2165/cm in the spectrum of L1551 IRS 5. New laboratory results over the 2200-2100/cm wavenumber interval, 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 through absorption bands at 2140/cm and 2135/cm. The relative abundance of solid state CO to frozen H2O is about 0.13 while the abundance of XCN seems comparable to that of frozen CO.
Document ID
19930057627
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Tegler, Stephen C.
(Notre Dame Univ. IN, United States)
Weintraub, David A.
(Vanderbilt Univ. Nashville, TN, United States)
Allamandola, Louis J.
(NASA Ames Research Center Moffett Field, CA, United States)
Sandford, Scott A.
(NASA Ames Research Center Moffett Field, CA, United States)
Rettig, Terrence W.
(Notre Dame Univ. IN, United States)
Campins, Humberto
(Florida Univ. Gainesville, United States)
Date Acquired
August 16, 2013
Publication Date
July 1, 1993
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 411
Issue: 1
ISSN: 0004-637X
Subject Category
Astrophysics
Accession Number
93A41624
Funding Number(s)
PROJECT: RTOP 199-52-12-04
Distribution Limits
Public
Copyright
Other

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