Zobrazeno 1 - 7
of 7
pro vyhledávání: '"Blustin, Alexander J."'
Autor:
Mehdipour, Missagh, Branduardi-Raymont, Graziella, Kaastra, Jelle S., Petrucci, Pierre-Olivier, Kriss, Gerard A., Ponti, Gabriele, Blustin, Alexander J., Paltani, Stephane, Cappi, Massimo, Detmers, Rob G., Steenbrugge, Katrien C.
We present the analysis of XMM-Newton and Swift optical-UV and X-ray observations of the Seyfert-1/QSO Mrk 509, part of an unprecedented multi-wavelength campaign, investigating the nuclear environment of this AGN. The XMM-Newton data are from a seri
Externí odkaz:
http://arxiv.org/abs/1107.0659
Autor:
Brown, Peter J., Dessart, Luc, Holland, Stephen T., Immler, Stefan, Landsman, Wayne, Blondin, Stephane, Blustin, Alexander J., Breeveld, Alice, Dewangan, Gulab C., Gehrels, Neil, Hutchins, Robert B., Kirshner, Robert P., Mason, Keith O., Mazzali, Paolo A., Milne, Peter, Modjaz, Maryam, Roming, Peter W. A.
Publikováno v:
Astrophys.J.659:1488-1495,2007
We report early photospheric-phase observations of the Type IIP Supernova (SN) 2005cs obtained by Swift's Ultraviolet-Optical and X-Ray Telescopes. Observations started within two days of discovery and continued regularly for three weeks. During this
Externí odkaz:
http://arxiv.org/abs/astro-ph/0612541
Autor:
McGowan, Katherine E., Charles, Phil A., Blustin, Alexander J., Livio, Mario, O'Donoghue, Darragh, Heathcote, Bernard
Publikováno v:
Mon.Not.Roy.Astron.Soc.364:462-474,2005
The highly luminous (> 10^37 erg s^-1) supersoft X-ray sources (SSS) are believed to be Eddington limited accreting white dwarfs undergoing surface hydrogen burning. The current paradigm for SSS involves thermally unstable mass transfer from a 1-2 so
Externí odkaz:
http://arxiv.org/abs/astro-ph/0509136
Autor:
Behar, Ehud, Rasmussen, Andrew P., Blustin, Alexander J., Sako, Masao, Kahn, Steven M., Kaastra, Jelle S., Branduardi-Raymont, Graziella, Steenbrugge, Katrien C.
Publikováno v:
Astrophys.J.598:232-241,2003
A long 280 ks observation of the Seyfert 1 galaxy NGC 3783 with XMM-Newton is reported. We focus on the oxygen line complex between 17 and 24 A as measured with the RGS spectrometers. Accurate absorption column densities and emission line fluxes are
Externí odkaz:
http://arxiv.org/abs/astro-ph/0307467
Autor:
Blustin, Alexander J.
Publikováno v:
Philosophical Transactions: Mathematical, Physical and Engineering Sciences, 2007 May . 365(1854), 1263-1268.
Externí odkaz:
https://www.jstor.org/stable/25190512
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Autor:
Brown, Peter J., Dessart, Luc, Holland, Stephen T., Immler, Stefan, Landsman, Wayne, Blondin, Stéphane, Blustin, Alexander J., Breeveld, Alice, Dewangan, Gulab C., Gehrels, Neil, Hutchins, Robert B., Kirshner, Robert P., Mason, Keith O., Mazzali, Paolo A., Milne, Peter, Modjaz, Maryam, Roming, Peter W. A.
Publikováno v:
Astrophysical Journal; 4/20/2007, Vol. 659 Issue 2, p1488-1495, 8p