dc.contributor.author |
Dewangan, G. C |
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dc.contributor.author |
Singh, K. P |
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dc.contributor.author |
Jones, L. R |
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dc.contributor.author |
McHardy, I. M |
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dc.contributor.author |
Newsam, A. M |
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dc.contributor.author |
Mason, K. O |
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dc.date.accessioned |
2008-05-13T09:48:14Z |
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dc.date.available |
2008-05-13T09:48:14Z |
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dc.date.issued |
2001 |
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dc.identifier.citation |
BASI, Vol. 29, No. 3, pp. 417 - 420 |
en |
dc.identifier.uri |
http://hdl.handle.net/2248/2294 |
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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 |
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dc.format.mimetype |
application/pdf |
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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 |
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dc.subject |
Galaxies:nuclei |
en |
dc.subject |
X-rays:galaxies |
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dc.title |
Discovery of a new NLQSO: RX J1334.2+3759 |
en |
dc.type |
Article |
en |