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Young stellar objects detected by IRASFluxes of 453 IRAS point sources selected for proximity to dense gas have been accurately determined by co-adding IRAS data. From this set, 258 sources are detected in all four bands: 12, 25, 60, and 100 microns. As distance from dense molecular material increases, these sources exhibit systematic trends in color and a markedly decreasing luminosity. These trends are broadly consistent with expected evolutionary changes in these stars, with younger objects found closer to dense gas. These data suggest a subtle variation on the criterion for identifying the youngest objects detectable by IRAS, in addition to that of steeply rising spectra: a color temperature which is uniform across all four IRAS bands in the range 40-50 K. These characteristics are used as a criterion to select point sources as candidate very young pre-main-sequence stars.
Document ID
19910049090
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Clark, Frank O.
(USAF, Geophysics Laboratory, Hanscom AFB MA, United States)
Date Acquired
August 14, 2013
Publication Date
February 1, 1991
Publication Information
Publication: Astrophysical Journal Supplement Series
Volume: 75
ISSN: 0067-0049
Subject Category
Astronomy
Report/Patent Number
ISSN: 0067-0049
Accession Number
91A33713
Funding Number(s)
CONTRACT_GRANT: NAG5-1184
Distribution Limits
Public
Copyright
Other

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