| dc.contributor.author | Dewangan, G. C | |
| dc.contributor.author | Singh, K. P | |
| dc.contributor.author | Jones, L. R | |
| dc.contributor.author | McHardy, I. M | |
| dc.contributor.author | Newsam, A. M | |
| dc.contributor.author | Mason, K. O | |
| dc.date.accessioned | 2008-05-13T09:48:14Z | |
| dc.date.available | 2008-05-13T09:48:14Z | |
| dc.date.issued | 2001 | |
| dc.identifier.citation | BASI, Vol. 29, No. 3, pp. 417 - 420 | en |
| dc.identifier.uri | http://hdl.handle.net/2248/2294 | |
| dc.description.abstract | A new narrow-line QSO, RX J1334.2+3759, has been identified at a redshift of 0.3858. The QSO has intrinsic soft X-ray luminosity ~ 2.8 x 1044 erg s-1. Soft X-ray emission from the QSO is highly variable. Rapid variability (change in intensity by a factor of ~ 4 within ~ 400 s) has also been found. The soft X-ray spectra of the QSO is well described by a power-law of photon index, ?x ~ 3.8. The optical spectrum of RX J1334.2+3759 is typical of narrow-line Seyfert 1 galaxies. The NLR of RX J1334.2+3759 appears to be significantly different from those of normal Seyfert 1 galaxies. | en |
| dc.format.extent | 343906 bytes | |
| dc.format.mimetype | application/pdf | |
| dc.language.iso | en | en |
| dc.publisher | Astronomical Society of India | en |
| dc.relation.uri | http://adsabs.harvard.edu/abs/2001BASI...29..417D | en |
| dc.subject | Galaxies:active | en |
| dc.subject | Galaxies:nuclei | en |
| dc.subject | X-rays:galaxies | en |
| dc.title | Discovery of a new NLQSO: RX J1334.2+3759 | en |
| dc.type | Article | en |