NIR spectroscopic observations of the SGR 1900+14 M stars

Details NIR spectroscopic observations of the SGR 1900+14 M stars NIR spectroscopic observations of the SGR 1900+14 M stars

Sep 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aipc..526..825g&link_type=abstract

GAMMA-RAY BURSTS: 5th Huntsville Symposium. AIP Conference Proceedings, Volume 526, pp. 825-829 (2000).

Physics

1

Mass Loss And Stellar Winds, Supergiant Stars, Neutron Stars, Jets And Bursts, Galactic Winds And Fountains

Scientific paper

We report on medium-resolution near-infrared spectroscopic observations
of the M5 super-giant binary that may be related to the Soft Gamma
Repeater SGR 1900+14. The observations were performed with CGS4 at UKIRT
and cover the wavelength range from 1.9 to 2.5 μm. .

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