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Millimeter and infrared observations of SGR 1806-20 (1995)

Wallyn, P. ; Mahoney, W. A. ; Corbel, S. ; [et al.]

Springer

Astrophysics and space science 231 (1995), S. 89-92

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ISSN: 1572-946X

Keywords: Gamma-ray:Bursts ; ISM:Individual (G10.0-0.3) ; Supernova remnants

Source: Springer Online Journal Archives 1860-2000

Topics: Physics

Notes: Abstract 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.

Type of Medium: Electronic Resource

URL: http://dx.doi.org/10.1007/BF00658594

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