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Infrared observations of anonymous IRC sourcesInfrared (0.9 to 18 microns) observations of 232 anonymous 2-micron Sky survey (IRC) sources are reported. Most of the objects appear to be late-type stars with little or no long-wave excess. About ten percent exhibit large excesses. Thirty-one of the brightest 11-micron sources have been remeasured to determine variability. These brighter objects appear to fall into two groups; one group resembles NML Tauri, while the other is like NML Cygni.
Document ID
19740054505
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Strecker, D. W.
(Minnesota, University, Minneapolis, Minn.; NASA, Ames Research Center Space Sciences Div., Moffett Field, Calif., United States)
Ney, E. P.
(Minnesota, University Minneapolis, Minn., United States)
Date Acquired
August 7, 2013
Publication Date
July 1, 1974
Publication Information
Publication: Astronomical Journal
Volume: 79
Subject Category
Space Sciences
Accession Number
74A37255
Funding Number(s)
CONTRACT_GRANT: NGL-24-005-008
Distribution Limits
Public
Copyright
Other

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