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| Query : 1995A&A...297L..67G |
1995A&A...297L..67G - Astronomy and Astrophysics, volume 297L67-70 (1995/5-2)
ROSAT observations of GRO J1655-40.
GREINER J., PREDEHL P. and POHL M.
Abstract (from CDS):
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.
Abstract Copyright: ∼
Journal keyword(s): X-ray transients - superluminal motion - X-ray binaries - black hole candidates - individual: GRO J1655-40
Simbad objects: 3
| Number of rows : 3 |
| N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2026 |
#notes |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | V* V1033 Sco | HXB | 16 54 00.1423963019 | -39 50 44.761701340 | 16.14 | F3-6IV | 1980 | 0 | ||||
| 2 | SS 433 | HXB | 19 11 49.5647697480 | +04 58 57.827127648 | 16.854 | 14.643 | A7Ib | 2253 | 4 | |||
| 3 | Granat 1915+105 | HXB | 19 15 11.55576 | +10 56 44.9052 | ~ | 2810 | 0 |
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