Zobrazeno 1 - 10
of 64
pro vyhledávání: '"L. Boirin"'
Autor:
M. Diaz Trigo, L. Boirin
Publikováno v:
Astronomische Nachrichten. 337:368-374
In the last decade, X-ray spectroscopy has enabled a wealth of discoveries of photoionised absorbers in X-ray binaries. Studies of such accretion disc atmospheres and winds are of fundamental importance to understand accretion processes and possible
Publikováno v:
Proceedings of the International Astronomical Union. 8:25-28
We discuss the variability of winds in two low-mass X-ray binaries, GX 13+1 and 4U 1630-47. XMM-Newton observations of these sources show that strong, photoionised winds with column densities well above 1022 cm−2 can be present in both neutron star
Publikováno v:
Astronomy & Astrophysics. 493:145-157
We have analysed data from five XMM-Newton observations of XB 1254-690, one of them simultaneous with INTEGRAL, to investigate the mechanism responsible for the highly variable dip durations and depths seen from this low-mass X-ray binary. Deep dips
Autor:
Mariano Mendez, Erik Kuulkers, Walter H. G. Lewin, Frits Paerels, Jean Cottam, L. Boirin, Jon M. Miller
Publikováno v:
The Astrophysical Journal. 672:504-509
Gravitationally redshifted absorption lines from highly ionized iron have been previously identified in the burst spectra of the neutron star in EXO 0748-676. To repeat this detection we obtained a long, nearly 600 ks observation of the source with X
Publikováno v:
Astronomy & Astrophysics. 445:179-195
X-ray observations have revealed that many microquasars and low-mass X-ray binaries (LMXBs) exhibit narrow absorption features identified with resonant absorption from Fe XXV and Fe XXVI and other abundant ions. In many well studied systems there is
Publikováno v:
Astronomy & Astrophysics. 436:195-208
We report the detection of narrow Fe XXV and Fe XXVI X-ray absorption lines at 6.68 +/- 0.04 keV and 6.97 +/- 0.05 keV in the persistent emission of the dipping low-mass X-ray binary 4U 1323-62 during a 2003 January XMM-Newton observation. These feat
Publikováno v:
Nuclear Physics B - Proceedings Supplements. 132:506-511
We report the discovery of narrow X-ray absorption features from the two dipping low-mass X-ray binary 4U 1916-053 and X 1254-690 during XMM-Newton observations. The features detected are identified with resonant scattering absorption lines of highly
Autor:
Finn Erland Christensen, Ersin Gogus, Katja Pottschmidt, Fiona A. Harrison, Chryssa Kouveliotou, Felix Fürst, John A. Tomsick, Walter Craig, Jon M. Miller, C. J. Hailey, Nathalie Degenaar, L. Boirin, S. E. Boggs, Allyn F. Tennant, Varun Bhalerao, Brian W. Grefenstette, George Younes, Andrew C. Fabian, Mark H. Finger, Poshak Gandhi, Deepto Chakrabarty, William W. Zhang, J. A. Kennea, Daniel Stern
Publikováno v:
Younes, G, Kouveliotou, C, Grefenstette, B W, Tomsick, J A, Tennant, A, Finger, M H, Fürst, F, Pottschmidt, K, Bhalerao, V, Boggs, S E, Christensen, F E & Miller, J M 2015, ' Simultaneous NuSTAR/Chandra Observations of The Bursting Pulsar GRO J1744-28 During Its Third Reactivation ', Astrophysical Journal, vol. 804, no. 1, 43 . https://doi.org/10.1088/0004-637X/804/1/43
We report on a 10 ks simultaneous Chandra/HETG-NuSTAR observation of the Bursting Pulsar, GRO J1744-28, during its third detected outburst since discovery and after nearly 18 years of quiescence. The source is detected up to 60 keV with an Eddington
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::58b88dfa2bd8c04740ba5ce7be67b341
https://resolver.caltech.edu/CaltechAUTHORS:20150605-135807207
https://resolver.caltech.edu/CaltechAUTHORS:20150605-135807207
Autor:
L. Boirin, Maria Diaz Trigo
Publikováno v:
Acta Polytechnica, Vol 53, Iss A (2013)
We review the current status of studies of disc atmospheres and winds in low mass X-ray binaries. We discuss the possible wind launching mechanisms and compare the predictions of the models with the existent observations. We conclude that a combinati
Publikováno v:
Advances in Space Research. 25:383-386
The type I X-ray burster 1E1724-3045 located in the globular cluster Terzan 2 was observed by the Rossi X-ray Timing Explorer (RXTE) while it was in a Island state, displaying both intense flickering and a hard Comptonized spectrum. No statistically