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Active star formation in NGC 2264The region of NGC 2264 near the cone nebula is the site of active star formation in a rotating ring seen nearly edge on as a two lobed source. Allen's infrared source (IRS 1) surrounds a B3V star still embedded in the southern lobe of the cloud. The northern lobe, IRS 2, also probably contains young stars.
Document ID
19850053276
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1086/163152
Authors
Schwartz, P. R. (U.S. Navy, E. O. Hulburt Center for Space Research, Washington DC, United States)
Thronson, H. A., Jr. (Wyoming Infrared Observatory Laramie, WY, United States)
Odenwald, S. F. (U.S. Navy, E. O. Hulburt Center for Space Research, Washington, DC; Sachs/Freeman Associates, Bowie MD, United States)
Glaccum, W. (Hulburt (E. O.) Center for Space Research Washington, DC, United States)
Loewenstein, R. F. (Yerkes Observatory Williams Bay, WI, United States)
Wolf, G. (Steward Observatory Tucson, AZ, United States)
Date Acquired
August 12, 2013
Publication Date
May 1, 1985
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 292
ISSN: 0004-637X
Subject Category
Astrophysics
Accession Number
85A35427
Funding Number(s)
CONTRACT_GRANT: NAG2-134
Distribution Limits
Public
Copyright
Other

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