ASCA Observations of Two SGRs: SGR 1806-20 and SGR 0526-66

Details ASCA Observations of Two SGRs: SGR 1806-20 and SGR 0526-66 ASCA Observations of Two SGRs: SGR 1806-20 and SGR 0526-66

Sep 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.231...57m&link_type=abstract

Astrophysics and Space Science, Volume 231, Issue 1-2, pp. 57-63

Astronomy and Astrophysics

Astrophysics

3

Soft Gamma-Ray Repeaters

Scientific paper

ASCA has observed two Soft Gamma-ray burst Repeaters (SGRs) among three known. This is a short report of the two SGRs, 1806 20 and 0526 66(N49). The observed X-ray characteristics favor a spin-powered system for SGR1806-20 and no ASCA detection of the hard X-ray component from SGR0526 66 suggests a very soft spectrum of the ROSAT HRI X-ray point source.

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