Brackett-gamma-line observations of G45.13 + 0.14A

Details Brackett-gamma-line observations of G45.13 + 0.14A Brackett-gamma-line observations of G45.13 + 0.14A

Nov 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985pasp...97.1112t&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 97, Nov. 1985, p. 1112-1114. Sponsorship: Ministry of E

Astronomy and Astrophysics

Astronomy

3

H Gamma Line, Hydrogen Clouds, Infrared Astronomy, Nebulae, Radio Sources (Astronomy), Spectral Line Width, Astronomical Spectroscopy, Early Stars, Ionized Gases, Stellar Winds

Scientific paper

Velocity-resolved observations of G 45.13+0.14A revealed that the Bγ(2.17 μm) emission line shows a peak velocity of 100±10 km s-1(LSR) and a deconvolved width of 100±15 km s-1(FWHM). Such a broad width was first detected for a highly luminous young stellar object. This width suggests that dense ionized gas flows outward from the central object.

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