Millimeter and Infrared Observations of SGR 1806-20

Details Millimeter and Infrared Observations of SGR 1806-20 Millimeter and Infrared Observations of SGR 1806-20

Sep 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.231...89w&link_type=abstract

Astrophysics and Space Science, Volume 231, Issue 1-2, pp. 89-92

Astronomy and Astrophysics

Astrophysics

7

Gamma-Ray:Bursts, Ism:Individual (G10.0-0.3), Supernova Remnants

Scientific paper

We present CO(1-0) observations toward the soft gamma-ray repeater SGR 1806-20. We discuss the implications on the distance to the X-ray counterpart: AX 1805.7-2025. We also present an upper limit at λ = 1.3 mm for the thermal emission from dust and high resolution IRAS maps of the region. SGR 1806-20 is very likely associated with the H II complex W31. The G10.0-0.3 supernova remnant (SNR) could be expanding in the very low density region produced by the wind of the bright O9-B2 star recently detected.

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