X-ray binaries are a class of binary stars that are luminous in X-rays. The X-rays are produced by matter falling from one component, called the donor... 14 KB (1,706 words) - 13:09, 1 May 2024 |
Be/X-ray binaries (BeXRBs) are a class of high-mass X-ray binaries that consist of a Be star and a neutron star. The neutron star is usually in a wide... 6 KB (874 words) - 23:29, 22 April 2024 |
intensity. The X-ray periods range from as little as a fraction of a second to as much as several minutes. An X-ray pulsar is a type of binary star system... 8 KB (1,073 words) - 15:08, 12 April 2024 |
Neutron star (redirect from Binary neutron stars) Intermediate-mass X-ray binary pulsars: a class of intermediate-mass X-ray binaries (IMXB), a pulsar with an intermediate mass star. High-mass X-ray binary pulsars:... 110 KB (13,299 words) - 13:20, 11 May 2024 |
List of neutron stars (section Anomalous X-ray pulsars) CXJ0110-7211 Vela X-1 4U 0352+309 Bursting Pulsar Vela Junior LMC N49 Intermediate-mass X-ray binary High-mass X-ray binaries Centaurus X-3 Circinus X-1 GX 301-2... 7 KB (452 words) - 19:51, 9 February 2024 |
Cygnus X-3 is a high-mass X-ray binary (HMXB), one of the stronger binary X-ray sources in the sky. It is often considered to be a microquasar, and it... 13 KB (1,455 words) - 06:33, 26 November 2023 |
}\ K^{3}}{2\pi G}}\left(1-e^{2}\right)^{3/2}.} If the accretor in an X-ray binary has a minimum mass that significantly exceeds the Tolman–Oppenheimer–Volkoff... 19 KB (2,239 words) - 22:58, 22 October 2023 |
erg/s. Super soft X-rays are believed to be produced by steady nuclear fusion on a white dwarf's surface of material pulled from a binary companion, the... 20 KB (2,508 words) - 01:33, 28 November 2023 |
X-rays from stellar sources in our galaxy were primarily from a neutron star in a binary system with a normal star. In these "X-ray binaries," the X-rays... 55 KB (7,174 words) - 21:14, 13 May 2024 |
Large Magellanic Cloud (section X-ray sources) LMC X-ray binaries: LMC X-1, X-2, X-3, X-4 and A 0538–66 (detected by Ariel 5 at A 0538–66), LMC X-2 is the one that is a bright low-mass X-ray binary system... 33 KB (3,563 words) - 01:01, 7 May 2024 |
XTE J1118+480 (category X-ray binaries) XTE J1118+480 is a low-mass X-ray binary in the constellation Ursa Major. It is a soft X-ray transient that most likely contains a black hole and is probably... 7 KB (696 words) - 06:10, 15 January 2024 |
magnetic field in universe directly detected by X-ray space observatory". phys.org. "Ultra-bright X-ray source awakens near a galaxy not so far away".... 3 KB (63 words) - 18:29, 11 March 2022 |
X-ray star may refer to: Be/X-ray binary, a class of high-mass X-ray binaries that consist of a Be star and a neutron star X-ray binary, a class of binary... 557 bytes (127 words) - 02:06, 18 December 2018 |
PSR J0952–0607 (category X-ray binaries) high-energy solar winds and gamma-ray emissions. The pulsar's high-energy emissions have been detected in gamma-ray and X-ray wavelengths. PSR J0952–0607 was... 19 KB (1,694 words) - 15:53, 2 May 2024 |
Mark T. (2022), "The Disk Veiling Effect of the Black Hole Low-mass X-Ray Binary A0620-00", The Astrophysical Journal, 925 (1): 83, arXiv:2112.07842,... 10 KB (978 words) - 20:30, 17 April 2024 |
Hercules X-1 (Her X-1), also known as 4U1656+35, is a moderately strong X-ray binary source first studied by the Uhuru satellite. It is composed of a... 8 KB (820 words) - 18:54, 24 October 2023 |
stars currently known. The constellation is also home to Cygnus X-1, a distant X-ray binary containing a supergiant and unseen massive companion that was... 51 KB (5,881 words) - 23:59, 1 May 2024 |
Scorpius X-1 is an X-ray source located roughly 9000 light years away in the constellation Scorpius. Scorpius X-1 was the first extrasolar X-ray source... 10 KB (1,101 words) - 01:36, 15 September 2023 |
X-ray binaries. Using the Chandra X-ray Observatory, Lewin and his graduate student David Pooley made extensive studies of supernovae and faint X-ray... 34 KB (3,634 words) - 22:43, 5 May 2024 |
Soft X-ray transients (SXTs), also known as X-ray novae and black hole X-ray transients, are composed of a compact object (most commonly a black hole... 7 KB (913 words) - 20:40, 14 January 2024 |
X-1 is a pulsing, eclipsing high-mass X-ray binary (HMXB) system, associated with the Uhuru source 4U 0900-40 and the supergiant star HD 77581. The X-ray... 7 KB (521 words) - 04:01, 25 February 2023 |