Far-infrared line and continuum observations of G0. 095 + 0. 012 and the E2 thermal radio filament near the Galactic center

Measurements 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 qual...

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Veröffentlicht in:	The Astrophysical journal 1991-04, Vol.370
Hauptverfasser:	Erickson, E.F., Haas, M.R., Colgan, S.W.J., Simpson, J.P., Rubin, R.H.
Format:	Artikel
Sprache:	eng
Schlagworte:	640105 - Astrophysics & Cosmology- Galaxies CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS ELECTROMAGNETIC RADIATION FAR INFRARED RADIATION GALAXIES GALAXY NUCLEI INFRARED RADIATION INFRARED SPECTRA MILKY WAY MORPHOLOGY RADIATIONS RADIOWAVE RADIATION SPECTRA STARS
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Zusammenfassung:	Measurements 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. 33 refs.
ISSN:	0004-637X 1538-4357
DOI:	10.1086/185979