Far-infrared line and continuum observations of G0.095 + 0.012 and the E2 thermal radio filament near the Galactic center

Details Far-infrared line and continuum observations of G0.095 + 0.012 and the E2 thermal radio filament near the Galactic center Far-infrared line and continuum observations of G0.095 + 0.012 and the E2 thermal radio filament near the Galactic center

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...370l..69e&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 370, April 1, 1991, p. L69-L72.

Astronomy and Astrophysics

Astronomy

42

Far Infrared Radiation, Galactic Nuclei, Infrared Sources (Astronomy), Milky Way Galaxy, Radio Emission, Continuous Radiation, Infrared Spectra, Line Spectra, Radio Spectra

Scientific paper

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.

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