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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 GO.095 + 0.012 and the E2 thermal 'arched' radio filament near the Galactic center are well explained by numerous embedded stars with T(sub eff) approximately 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
19970020042
Acquisition Source
Ames Research Center
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)
Colgan, Sean W. J. (NASA Ames Research Center Moffett Field, CA United States)
Simpson, J. P. (NASA Ames Research Center Moffett Field, CA United States)
Rubin, Robert H. (NASA Ames Research Center Moffett Field, CA United States)
Morris, Mark (California Univ. Los Angeles, CA United States)
Haas, Michael R. (NASA Ames Research Center Moffett Field, CA United States)
Date Acquired
August 17, 2013
Publication Date
April 1, 1991
Publication Information
Publication: The Astrophysical Journal
Publisher: The American Astronomical Society
Volume: 370
Subject Category
Astronomy
Report/Patent Number
NAS 1.26:204208
NASA-CR-204208
Accession Number
97N71919
Funding Number(s)
CONTRACT_GRANT: NCC2-548
CONTRACT_GRANT: NCA2-373
CONTRACT_GRANT: NCC2-647
Distribution Limits
Public
Copyright
Public Use Permitted.
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