ROSAT observations of GRO J1655-40

Details ROSAT observations of GRO J1655-40 ROSAT observations of GRO J1655-40

May 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995a%26a...297l..67g&link_type=abstract

Astronomy and Astrophysics, v.297, p.L67

Astronomy and Astrophysics

Astrophysics

19

X-Ray Transients, Superluminal Motion, X-Ray Binaries, Black Hole Candidates, Gro J1655-40

Scientific paper

We have observed GRO J1655-40 with the ROSAT HRI between the first two
of the three outbursts in 1994. Besides improving the X-ray position we
derive a distance of d=~3kpc from the dust scattering halo. Combination
with radio measurements suggest that the X-ray emission originates in an
accretion disk or corona rather then in a jet.

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