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Far-infrared line and continuum observations of G0.095 + 0.012 and the E2 thermal radio filament near the Galactic centerMeasurements of far-infrared lines and continuum from G0.095 + 0.012 and the E2 thermal 'arched' radio filament near the Galactic center are well explained by numerous embedded stars with T(eff) about 35,000 K. The structure of the filament and the apparent absence of hotter stars are qualitatively difficult to reconcile with this idea.
Document ID
19910044062
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1086/185979
Authors
Erickson, Edwin F. (NASA Ames Research Center Moffett Field, CA, United States)
Haas, Michael R. (NASA Ames Research Center Moffett Field, CA, United States)
Colgan, Sean W. J. (NASA Ames Research Center; SETI Institute Moffett Field, CA, United States)
Simpson, J. P. (NASA Ames Research Center Moffett Field; California, University, Berkeley, United States)
Rubin, Robert H. (NASA Ames Research Center Moffett Field; California, University, Los Angeles, United States)
Date Acquired
August 14, 2013
Publication Date
April 1, 1991
Publication Information
Publication: Astrophysical Journal, Part 2 - Letters
Volume: 370
ISSN: 0004-637X
Subject Category
Astrophysics
Accession Number
91A28685
Funding Number(s)
CONTRACT_GRANT: NCA2-373
CONTRACT_GRANT: NCC2-548
CONTRACT_GRANT: NCC2-647
Distribution Limits
Public
Copyright
Other

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