Issue |
A&A
Volume 433, Number 2, April II 2005
|
|
---|---|---|
Page(s) | 515 - 518 | |
Section | Extragalactic astronomy | |
DOI | https://doi.org/10.1051/0004-6361:20042353 | |
Published online | 22 March 2005 |
Investigating the EGRET-radio galaxies link with INTEGRAL: The case of 3EG J1621+8203 and NGC 6251*
1
Istituto di Astrofisica Spaziale e Fisica Cosmica (IASF) del CNR/INAF, Sezione di Bologna, via Gobetti 101, 40129 Bologna, Italy e-mail: foschini@bo.iasf.cnr.it
2
Istituto di Radioastronomia (IRA) del CNR/INAF, via Gobetti 101, 40129 Bologna, Italy
3
Université Paris VII Denis-Diderot, 2 place Jussieu, 75251 Paris Cedex 05, France
4
CEA Saclay, DSM/DAPNIA/SAp (CNRS FRE 2591), 91191 Gif-sur-Yvette Cedex, France
5
XMM-Newton SOC - European Space Astronomy Center of ESA, Vilspa, Apartado 50727, 28080 Madrid, Spain
6
SRON National Institute for Space Research, Sorbonnelaan 2, 3584 CA Utrecht, The Netherlands
7
Astronomical Institute “Anton Pannekoek”, University of Amsterdam, Kruislaan 403, 1098 SJ Amsterdam, The Netherlands
8
Dipartimento di Astronomia, Università di Bologna, via Ranzani 1, 40127 Bologna, Italy
9
INTEGRAL Science Data Centre, Chemin d'Écogia 16, Versoix, Switzerland
Received:
10
November
2004
Accepted:
6
December
2004
The analysis of an INTEGRAL AO2 observation of the error contours
of the EGRET source 3EG J1621+8203 is presented. The only
source found inside the error contours for energies between 20 and 30 keV at detection significance is the FR I radio galaxy
NGC 6251. This supports the identification of NGC 6251 with 3EG J1621+8203.
The observed flux is higher and softer than observed
in the past, but consistent with a variable blazar-like spectral energy distribution.
Key words: X-rays: galaxies / galaxies: active / galaxies: individual: NGC 6251
© ESO, 2005
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