Results 1 to 10 of about 71,430 (133)
Six new candidate ultracompact X-ray binaries [PDF]
, 2007 Ultracompact X-ray binaries (UCXBs) appear able to sustain accretion onto the
compact accretor at rates lower than in wider X-ray binaries. This may be
understood by the smaller accretion disks in UCXBs: a lower X-ray luminosity
suffices to keep a disk ...Barret, Bassa, Bird, Burrows, C. B. Markwardt, Chelovekov, Chevalier, Cocchi, Cocchi, Cocchi, Cornelisse, Cornelisse, Cornelisse, Cumming, Cumming, Deloye, Deutsch, Dickey, Dieball, Dubus, Elvis, Fabian, Fujimoto, Fujimoto, Galloway, Galloway, Haggard, Hakala, Heinke, Heinke, Hoffman, Homer, Hoshi, Hynes, Iaria, in 't Zand, in 't Zand, in 't Zand, in 't Zand, in 't Zand, in 't Zand, J. J. M. in 't Zand, Jonker, Juett, Juett, Juett, Kaptein, Kirsch, Kuulkers, Kuulkers, Kuulkers, Lapidus, Levine, Lewin, Markwardt, Matsuba, Menou, Middleditch, Migliari, Molkov, Molkov, Mori, Nelemans, Nelemans, Nelson, Ortolani, Osaki, Osaki, P. G. Jonker, Parmar, Pavlinsky, Savonije, Schatz, Sidoli, Skinner, Skinner, Smak, Smale, Stella, Stephen, Swank, Tennant, van Paradijs, Van Paradijs, van Paradijs, Wang, Wen, Werner, White, White, Whitehurst, Wilson, Wolff, Woosley +93 morecore +2 more sourcesRelativistic outflow from two thermonuclear shell flashes on neutron
stars [PDF]
, 2014 We study the exceptionally short (32-41 ms) precursors of two
intermediate-duration thermonuclear X-ray bursts observed with RXTE from the
neutron stars in 4U 0614+09 and 2S 0918-549.Agrawal, Bartenev, Belian, Brandt, Cash, Cavecchi, Cornelisse, Cumming, Cumming, Cumming, Damen, Degenaar, Ebisuzaki, Feroci, Frolov, Fryxell, Fujimoto, Fujimoto, Galloway, Galloway, Giacconi, Grindlay, Grindlay, Hanawa, Heger, Heger, Hoffman, in’t Zand, in’t Zand, in’t Zand, in’t Zand, in’t Zand, in’t Zand, in’t Zand, in’t Zand, in’t Zand, J. J. M. in ’t Zand, Jager, Jahoda, Joss, Joss, Juett, Keek, Kuulkers, Kuulkers, Kuulkers, L. Keek, Lamb, Lewin, Lewin, London, Lund, Makhviladze, Molkov, Molkov, Nelemans, Nelemans, Nelson, Nobili, Paczynski, Pavlov, Rauscher, Rees, Shahbaz, Shaposhnikov, Simonenko, Spitkovsky, Strohmayer, Strohmayer, Suleimanov, Swank, Tawara, Tawara, van Paradijs, Wallace, Watts, Weaver, Weinberg, Weinberg, Woosley, Woosley, Worpel, Y. Cavecchi, Zel’Dovich, Zhong, Zingale +85 morecore +2 more sourcesIdentification of the optical and quiescent counterparts to the bright
X-ray transient in NGC 6440 [PDF]
, 2001 After 3 years of quiescence, the globular cluster NGC 6440 exhibited a bright
transient X-ray source turning on in August 2001, as noted with the RXTE
All-Sky Monitor.Asai K., D. Pooley, F. Verbunt, Guainazzi M., J. J. M. in ’t Zand, M. H. van Kerkwijk, Mitsuda K., Ortolani S., R. Wijnands, Verbunt F., W. H. G. Lewin, Zavlin V. E., ’t Zand J. J. M. +12 morecore +3 more sourcesOn the nature of two low M-dot X-ray bursters: 1RXS J170854.4-321857 and
1RXS J171824.2-402934 [PDF]
, 2005 We carried out Chandra observations of two low-luminosity low-mass X-ray
binaries, 1RXS J170854.4-321857 and 1RXS J171824.2-402934, for which previously
single X-ray bursts had been detected with the Wide Field Cameras (WFCs) on
board BeppoSAX. Both were Asai, Barret, Boella, Cocchi, Cornelisse, Cornelisse, Davis, Deloye, Dubus, Forman, Garmire, Hameury, Hands, Hoffman, J. J. M. in 't Zand, Jager, Jahoda, Jonker, Kaptein, Kuulkers, Levine, Lewin, Lin, Liu, M. Méndez, Markert, Menou, Menou, Motch, Muno, Piraino, R. Cornelisse, Revnivtsev, Rutledge, Tavani, van Paradijs, Van Paradijs, Verbunt, Wijnands, Wilson, Wood +40 morecore +1 more sourceAstrophysical parameters and orbital solution of the peculiar X-ray
transient IGR J00370+6122 [PDF]
, 2014 BD+6073 is the optical counterpart of the X-ray source IGR J00370+6122, a
probable accretion-powered X-ray pulsar. The X-ray light curve of this binary
system shows clear periodicity at 15.7 d, which has been interpreted as
repeated outbursts around the ...Castro, N., González-Galán, A., Lorenzo, J., Negueruela, I., Simón-Díaz, S., Vilardell, F. +5 morecore +3 more sourcesThe very faint hard state of the persistent neutron star X-ray binary
SLX 1737-282 near the Galactic centre [PDF]
, 2017 We report on a detailed study of the spectral and temporal properties of the
neutron star low mass X-ray binary SLX 1737-282, which is located only ~1degr
away from Sgr A.De Marco, B., Haberl, F., Muñoz-Darias, T., Padilla, M. Armas, Ponti, G. +4 morecore +2 more sourcesThe cooling rate of neutron stars after thermonuclear shell flashes [PDF]
, 2013 Thermonuclear shell flashes on neutron stars are detected as bright X-ray
bursts. Traditionally, their decay is modeled with an exponential function.
However, this is not what theory predicts.A. Cumming, Bradt, Clauset, Cumming, Cumming, Cumming, Fisker, Fujimoto, Galloway, Gudmundsson, Hanawa, Heger, in ’t Zand, in ’t Zand, J. J. M. in ’t Zand, Jahoda, Lampton, Lewin, Linares, London, Madej, Mitsuda, Morrison, Parmar, R. A. D. A. Mateijsen, Strohmayer, Suleimanov, T. Bagnoli, T. L. Triemstra, Wallace, Woosley, Worpel +31 morecore +1 more sourceX-ray variability during the quiescent state of the neutron-star X-ray
transient in the globular cluster NGC 6440 [PDF]
, 2004 The globular cluster NGC 6440 is known to harbor a bright neutron-star X-ray
transient. We observed the globular cluster with Chandra on two occasions when
the bright transient was in its quiescent state in July 2000 and June 2003
(both observations were Craig O. Heinke, David Pooley, Edward M. Cackett, Jon M. Miller, Jonathan E. Grindlay, Ortolani S., Peter D. Edmonds, Peter G. Jonker, Rudy Wijnands, Verbunt F., Walter H. G. Lewin, Zavlin V. E., ’t Zand J., ’t Zand J. J. M. +13 morecore +3 more sourcesDiscovery of a large and bright bow shock nebula associated with low
mass X-ray binary SAX J1712.6-3739
, 2009 In a multiwavelength program dedicated to identifying optical counterparts of
faint persistent X-ray sources in the Galactic Bulge, we find an accurate X-ray
position of SAX J1712.6-3739 through Chandra observations, and discover its
faint optical ...A. M. Read, Allen, Chatterjee, Cocchi, Cooke, Corbel, Corbel, Cox, D. M. Russell, Fender, Fomalont, Gallo, Heinz, Heinz, In 't Zand, In 't Zand, K. Wiersema, M. Klein-Wolt, Malzac, Margon, Migliari, Migliari, N. Degenaar, N. R. Tanvir, Nelemans, Pakull, Parker, Predehl, R. D. Saxton, R. Wijnands, Russell, Russell, Russell, S. Heinz, Saxton, Shahbaz, Tingay, Tudose, Van Paradijs, Vrtilek, Witham +40 morecore +4 more sourcesDiscovery of the neutron star nature of SLX 1737-282
, 2002 SLX 1737-282 is a persistent moderately bright X-ray source 1.2 deg from the
Galactic center. X-ray observations with the Wide Field Cameras on BeppoSAX
have for the first time revealed the true nature of SLX 1737-282: a 15-min long
thermonuclear flash ...A. Bazzano, Boella, Boella, C. B. Markwardt, E. Kuulkers, Emelyanov, F. Verbunt, Frontera, Fujimoto, Hertz, J. Heise, J. J. M. in 't Zand, Jager, Jonker, Juett, Kaptein, Kitamoto, Kuulkers, Kuulkers, L. Natalucci, Lewin, Liu, M. Cocchi, Motch, P. Ubertini, Parmar, Pavlinsky, R. Cornelisse, Sakano, Skinner, Swank, Tawara, Van Paradijs +32 morecore +2 more sources
