dc.contributor.author |
Ghosh, K. K |
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dc.contributor.author |
Soundararajaperumal, S |
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dc.date.accessioned |
2008-07-02T11:03:32Z |
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dc.date.available |
2008-07-02T11:03:32Z |
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dc.date.issued |
1991-12 |
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dc.identifier.citation |
Astrophysical Journal, Part 1, Vol. 383, No. 2, pp. 574 - 579 |
en |
dc.identifier.issn |
0004-637X |
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dc.identifier.uri |
http://hdl.handle.net/2248/2576 |
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dc.description.abstract |
This study presents results of the X-ray spectra (0.1-10 keV) of the Seyfert galaxy NGC 3516 on the basis of Exosat observations obtained on four epochs between 1985/308 and 1985/340. The soft X-ray (0.2-2 keV) flux of this galaxy varied by a factor of about 3 on the time scales of 2 d, and that for the hard X-ray (2-10 keV) flux varied by a factor of about 1.5 over the period of a month. The observed spectra are best fitted by a power-law, uniform absorption, and a Gaussian line model. Best-fit parameters of this model suggest that NGC 3516 is a flat spectrum source. Weak soft excess and significant intrinsic absorption (about 10 exp 22/sq cm) were detected in the spectrum of this galaxy. An emission line detected with a high significance (greater than 99.9 percent) around 6.0 keV could be the redshifted 6.4-keV iron line due to the fluorescence of thick cold iron present around the nucleus of NGC 3516 or due to the redshifted 6.7-keV helium-like iron line produced in an optically thin hot plasma of temperature around 10 exp 8 K. |
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dc.format.extent |
925408 bytes |
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dc.format.mimetype |
application/pdf |
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dc.language.iso |
en |
en |
dc.publisher |
University of Chicago press |
en |
dc.relation.uri |
http://adsabs.harvard.edu/abs/1991ApJ...383..574G |
en |
dc.subject |
Exosat Satellite |
en |
dc.subject |
Seyfert galaxies |
en |
dc.subject |
X ray spectra |
en |
dc.subject |
Absorption spectra |
en |
dc.subject |
High temperature plasmas |
en |
dc.subject |
Red shift |
en |
dc.title |
EXOSAT observations of the Seyfert 1 galaxy NGC 3516 |
en |
dc.type |
Article |
en |