XMM-NEWTON Observation of the Seyfert 2 Galaxy NGC 4138
| dc.creator | Foschini, L. | |
| dc.creator | Panessa, F. | |
| dc.creator | Longinotti, A. L. | |
| dc.creator | Ho, L. C. | |
| dc.creator | Bassani, L. | |
| dc.creator | Cappi, M. | |
| dc.creator | Dadina, M. | |
| dc.creator | Malaguti, G. | |
| dc.creator | Di Cocco, G. | |
| dc.creator | Gianotti, F. | |
| dc.creator | Stephen, J. B. | |
| dc.creator | Trifoglio, M. | |
| dc.date | 2002-09-05 | |
| dc.date.accessioned | 2026-07-07T02:04:59Z | |
| dc.date.available | 2026-07-07T02:04:59Z | |
| dc.description | The XMM-Newton data presented here are the first X-ray observation of the Seyfert 2 galaxy NGC4138. Although the galaxy has been pointed by ROSAT-HRI, it was not detected, with a flux upper limit of about 1.1x10^-13 erg cm^-2 s^-1 in the 0.2-2.4 keV energy band. XMM-Newton performed the observation on 26 November 2001. The source is detected for the first time in X-rays with F[0.2-2.4]=1.0x10^-13 erg cm^-2 s^-1, in agreement with the upper limit of ROSAT. The source spectrum is typical of Seyfert 2 galaxies. We find heavy obscuration (N_H about 8x10^22 cm^-2) and a flat photon index (1.6). The source intrinsic luminosity is about 5x10^41 erg/s in the 0.5-10 keV energy band. | |
| dc.description | 4 pages, 3 figures. Presented at AGN05: Inflows, Outflows and Reprocessing around black holes, Como (Italy), 11-14 June 2002. To appear in the Proceedings. If you have problems in download, please check also this http://www.bo.iasf.cnr.it/~foschini/pub/0209098.ps.gz | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0209098 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0209098 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/4973 | |
| dc.subject | Astrophysics | |
| dc.title | XMM-NEWTON Observation of the Seyfert 2 Galaxy NGC 4138 | |
| dc.type | text |