ISOCAM preliminary results on the environmentof the Soft Gamma-ray Repeater SGR 1806-20

Details ISOCAM preliminary results on the environmentof the Soft Gamma-ray Repeater SGR 1806-20 ISOCAM preliminary results on the environmentof the Soft Gamma-ray Repeater SGR 1806-20

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998tx19.confe.236f&link_type=abstract

Abstracts of the 19th Texas Symposium on Relativistic Astrophysics and Cosmology, held in Paris, France, Dec. 14-18, 1998. Eds.:

Astronomy and Astrophysics

Astrophysics

Scientific paper

We have obtained ISOCAM images of SGR 1806-20 in the 5-18 microns range
with several LW large band filters: it may be associated with a young
star region. This assumption is compatible with the presence of an LBV
star which has been previously associated with SGR 1806-20. The physical
connection between these two objects is still not proved.

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