- Author
-
E. Kuulkers
S. Shaw
J. Chenevez
S. Brandt
A. Domingo
P. Kretschmar
C. Markwardt
N. Mowlavi
A. Paizis
D. Risquez
C. Sanchez-Fernandez
R. Wijnands - Year
- 2007
- Title
- IGR J17453-2853 = Granat 1741.9-2853?
- Journal
- The astronomer's telegram
- Volume
- 1008
- Pages (from-to)
- 1
- Document type
- Article
- Faculty
- Faculty of Science (FNWI)
- Institute
- Anton Pannekoek Institute for Astronomy (API)
- Abstract
-
The position of the recently found source IGR J17453-2853 as derived by INTEGRAL IBIS/ISGRI (see ATel #1005) is about 4 arcmin from that of Granat 1741.9-2853 (see ATel #1006; Muno et al. 2003, ApJ 598, 474). Formally, given the statistical 90% error regions of both sources (IGR J17453-2853: about 2 arcmin; Granat 1741.9-2853: about 1 arcsec), they can be regarded as two different sources. However, Granat 1741.9-2853 was found to be the only X-ray transient active in the near vicinity of IGR J17453-2853 by the Swift/XRT, about a day after the INTEGRAL observations (ATel #1006).
- Link
- Link
- Language
- Undefined/Unknown
- Persistent Identifier
- https://hdl.handle.net/11245/1.287598
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