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The infrared sources in M8.The spectral energy distribution and size of the source of infrared radiation from Herschel 36 in M8 have been investigated. Radiation from the diffuse source in the vicinity of the hourglass has been measured. It is shown that a significant fraction of the 10-microns flux comes from an unresolved source centered on Herschel 36. Other stars in M8 have also been investigated as potential sources of infrared radiation.
Document ID
19730036091
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1086/181128
Authors
Woolf, N. J. (Minnesota, University Minneapolis, Minn., United States)
Stein, W. A. (California, University Berkeley, Calif.; Minnesota, University, Minneapolis, Minn., United States)
Gillett, F. C.
Merrill, K. M. (California, University San Diego, Calif., United States)
Becklin, E. E.
Neugebauer, G. (Hale Observatories Pasadena, Calif., United States)
Pepin, T. J. (Wyoming, University Laramie, Wyo., United States)
Date Acquired
August 7, 2013
Publication Date
February 1, 1973
Publication Information
Publication: Astrophysical Journal
Volume: 179
Subject Category
Space Sciences
Accession Number
73A20893
Distribution Limits
Public
Copyright
Other

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