Searches , social queries for LOW MASS-X-RAY-BINARY
Search references for LOW MASS-X-RAY-BINARY. Phrases containing LOW MASS-X-RAY-BINARY
See searches and references containing LOW MASS-X-RAY-BINARY!
Search references for LOW MASS-X-RAY-BINARY. Phrases containing LOW MASS-X-RAY-BINARY
See searches and references containing LOW MASS-X-RAY-BINARY!LOW MASS-X-RAY-BINARY
Type of astronomical binary system
Low-mass X-ray binaries (LMXBs or LMXRBs) are X-ray binary systems containing a compact object, typically a neutron star or black hole, and a normal star
Low-mass_X-ray_binary
Class of binary stars
classification by mass (high, intermediate, low) refers to the optically visible donor, not to the compact X-ray emitting accretor. Low-mass X-ray binaries (LMXBs)
X-ray_binary
Type of binary star
A high-mass X-ray binary (HMXB or HMXRB) is a binary star system containing a compact object (typically a black hole or neutron star) and a normal star
High-mass_X-ray_binary
Class of high-mass X-ray binaries
Be/X-ray binaries (BeXRBs or BeXBs) 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
Be/X-ray_binary
Type of low-mass X-ray binary
bright low-mass X-ray binary (LMXB) containing a neutron star accreting off of another star. Atoll sources have relatively weak magnetic fields and low luminosities
Atoll_source
Low-mass X-ray binary
Cygnus X-2, also known as V1341 Cygni, is a low-mass X-ray binary (LMXB) containing a neutron star as the compact object. It is located in the constellation
Cygnus_X-2
Type of low-mass X-ray binary
of neutron star low-mass X-ray binary (LMXB) distinguishable from the similar atoll source by the characteristic "Z" shape of its X-ray color-color diagram
Z_source
Ultraluminous x-ray binary
Swift J1727.8-1613 (also known as J1727) is a ultraluminous low-mass x-ray binary 8,800 light years (2,698 parsecs) away with an orbital period of about
Swift_J1727.8−1613
X-ray Binary in the Large Magellanic Cloud
X-2 is a low-mass X-ray binary (LMXB) located in the Large Magellanic Cloud (LMC), a satellite galaxy of Milky Way. It is one of the five brightest X-ray
LMC_X-2
Collapsed core of a massive star
"accretion-powered pulsars": a class of X-ray binaries Low-mass X-ray binary pulsars: a class of low-mass X-ray binaries (LMXB), a pulsar with a main-sequence
Neutron_star
X-ray binary in Cygnus containing a stellar black hole
of the source region" of occasional X-ray bursts lasting only for about 1 ms. Cygnus X-1 is a high-mass X-ray binary system located about 7,000 light-years
Cygnus_X-1
Star system in the constellation Ursa Major
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
XTE_J1118+480
X-ray binary in the Large Magellanic Cloud
LMC X-3 is a high-mass X-ray binary (HMXB) system located in the Large Magellanic Cloud (LMC), a satellite galaxy of the Milky Way approximately 165,000
LMC_X-3
Astronomical X-ray source
Scorpius X-1 is a low-mass X-ray binary located roughly 9,000 light years away in the constellation Scorpius. Scorpius X-1 was the first extrasolar X-ray source
Scorpius_X-1
Low-mass X-ray binary in Carina
V395 Carinae, also known as 2S 0921-630, is a low-mass X-ray binary in the constellation Carina. X-ray observations have revealed that it has an extended
V395_Carinae
Satellite galaxy of the Milky Way
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
Large_Magellanic_Cloud
Class of X-ray binary stars
X-ray bursters are one class of X-ray binary stars exhibiting X-ray bursts, periodic and rapid increases in luminosity (typically a factor of 10 or greater)
X-ray_burster
X-ray Binary in Globular Cluster Messier 10
M10-VLA1 is a variable low-mass X-ray binary in the globular cluster Messier 10 that is also a radio source, situated in the equatorial constellation
M10-VLA1
Neutron star
3XMM J004232.1+411314 is a low-mass X-ray binary hosted in the galaxy M31. It is the most luminous source of hard X-rays in the Andromeda Galaxy. It is
3XMM_J004232.1+411314
X-ray binary
47 Tucanae X9 (also known as 47 Tuc X9) is an ultracompact low-mass X-ray binary (LMXB) located within the globular cluster 47 Tucanae, one of the brightest
47_Tucanae_X9
System of two stars orbiting each other
systems. In X-ray binaries, the compact object can be either a neutron star or a black hole. These binaries are classified as low-mass or high-mass according
Binary_star
Low mass X-ray binary in the constellation Volans
UY Volantis, also known as EXO 0748-676, is a low mass X-ray binary system located in the constellation Volans. With an apparent magnitude of 16.9, it
UY_Volantis
Star in the constellation Ophiuchus
(GRS 1716−249, V2293 Oph, X-Ray Nova Ophiuchi 1993) is believed to be a low-mass X-ray binary. Its name derives from an X-ray transient, detected in 1993
GRO_J1719−24
Star in the constellation Sagittarius
The Bursting Pulsar (GRO J1744-28) is a low-mass x-ray binary with a period of 11.8 days. It was discovered in December 1995 by the Burst and Transient
Bursting_Pulsar
Star in the constellation Musca
the incoming stream of material from the donor star. "GR Muscae – Low Mass X-ray Binary". SIMBAD Astronomical Database. Centre de Données astronomiques
GR_Muscae
Neutron star in the constellation Ophiuchus
XTE J1739−285 is a low-mass X-ray binary in the constellation Ophiuchus, situated approximately 13,000 light-years from Earth. It was first observed on
XTE_J1739−285
X-ray binary in the Large Magellanic Cloud
LMC X-4 is an eclipsing high-mass X-ray binary (HMXB) pulsar system located in the Large Magellanic Cloud (LMC), a satellite galaxy of the Milky Way approximately
LMC_X-4
Astronomical objects
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
List_of_neutron_stars
Low-mass X-ray binary star in the constellation Corona Borealis
6+2600, is a low-mass X-ray binary star system in the constellation Corona Borealis. Astronomer Simon Morris and colleagues discovered the X-ray source in
UW_Coronae_Borealis
Astronomical object emitting X-rays
the massive X-ray binaries although it falls on the borderline, ~2 M☉, between high- and low-mass X-ray binaries. The first extrasolar X-ray source was
Astrophysical_X-ray_source
High mass X-ray binary in the constellation of Cygnus
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
Cygnus_X-3
Class of millisecond pulsars
pulsars are a class of millisecond pulsars that occur in tight binary systems with a low-mass, non-degenerate companion, such as a star or substellar object
Spider_pulsar
Black hole formed by a collapsed star
September 2021). "Dynamical confirmation of a stellar mass black hole in the transient X-ray dipping binary MAXI J1305-704". Monthly Notices of the Royal Astronomical
Stellar_black_hole
Paradijs, J.; van den Heuvel, E.P.J. (July 2007), "A Catalogue of low-mass X-ray binaries in the Galaxy, LMC, and SMC (Fourth edition)", Astronomy and Astrophysics
List of nearest known black holes
List_of_nearest_known_black_holes
Active low mass X ray binary star
active low-mass X-ray binary in the constellation Norma. It is composed of a neutron star and a star smaller and cooler than the Sun. The X-ray component
QX_Normae
Binary Star in the constellation Hercules
Her X-1 is the prototype for the massive X-ray binaries although it falls on the borderline, ~2 M☉, between high- and low-mass X-ray binaries. An intermediate-mass
Hercules_X-1
Globular cluster
retrograde and prograde motion observed in the movement of its stars. Low mass X-ray binary 4U 1724-307 is also located in Terzan 2. Terzan Catalogue "Terzan
Terzan_2
Stellar-mass black hole in the constellation Sagittarius
J1745−26 in visible light. SWIFT J1745−26 must be a member of a low-mass X-ray binary (LMXB) system, which includes a normal, sun-like star. Roman, Nancy
SWIFT_J1745−26
Binary star in the constellation Orion
4U 0614+091 is a low-mass X-ray binary star system which features a neutron star and a low-mass companion star. The binary system lies 10,000 light-years
4U_0614+091
Massive millisecond pulsar in the Milky Way
have been detected in gamma-ray and X-ray wavelengths. PSR J0952−0607 was first identified as an unassociated gamma-ray source detected during the first
PSR_J0952−0607
Star in the constellation of Cygnus
rays emitted from WR 136's hot surface cause the shell to glow. There is some evidence WR 136 may be a binary star. Its companion would be a low-mass
WR_136
Dutch astrophysicist (born 1936)
neutron stars. In his search for millisecond X-ray pulsations from low-mass X-ray binaries, in 1984–85 Lewin made guest observations with the European observatory
Walter_Lewin
Class of astronomical objects that are X-ray sources
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
X-ray_pulsar
Binary star
the mass of the Sun. The optical companion of this low-mass X-ray binary is a subgiant F star. GRO J1655−40 was discovered by the Compton Gamma Ray Observatory
GRO_J1655−40
Globular cluster
sources, many of which are likely Low-mass X-ray binaries (LMXB) or cataclysmic variables. The large number of X-ray sources and millisecond pulsars may
Terzan_5
Star in the constellation Norma
a low-mass X-ray binary. The companion star would orbit in an elongated orbit. When the companion is close to the neutron star, it would feed mass into
1E_161348−5055
List of compact objects with mass of 2.5–5 solar masses
Paul A.; Robinson, Edward L. (2015). "The Case for a Low Mass Black Hole in the Low Mass X-Ray Binary V1408 Aquilae (= 4U 1957+115)". The Astrophysical Journal
List of lower mass gap objects
List_of_lower_mass_gap_objects
X-ray binary in the constellation Pegasus
combined with distance estimates, indicated it is consistent with a low-mass X-ray binary system containing a candidate black hole. The spectra displayed
MAXI_J1820+070
Star in the constellation Vulpecula
low-mass X-ray binary. List of nearest black holes Chevalier, C.; Ilovaisky, S. A. (March 1993). "Optical studies of transient low-mass X-ray binaries. IV
GS_2000+25
Double stars that show a significant interaction between their components
dwarf with a mass as low as 0.1 M☉. The same scenario works when the companion is a millisecond pulsar. Evolutionary models of binaries suggest that a
Interacting_binary_star
Ancient circumbinary jovian exoplanet orbiting PSR B1620-26 binary system
the stars formed a low-mass X-ray binary, as the infalling matter was heated to temperatures high enough to glow in X-rays. Mass transfer came to an
PSR_B1620−26_b
Star in the constellation Norma
sometimes abbreviated to J1550 and also known as V381 Normae, is a low-mass X-ray binary in the constellation Norma. It is composed of a black hole around
XTE_J1550−564
Branch of astronomy that uses X-ray observation
prototype for the massive X-ray binaries although it falls on the borderline, ~2 M☉, between high- and low-mass X-ray binaries. In July 2020, astronomers
X-ray_astronomy
Astronomic function
In astronomy, the binary mass function or simply mass function is a function that constrains the mass of the unseen component (typically a star or exoplanet)
Binary_mass_function
low-mass X-ray binary GX 340+0 16h 45m 47.7s −45° 36′ 40″ low-mass X-ray binary H1743-322 17h 46m 15.61s −32° 14′ 00.6″ low-mass X-ray binary OAO 1657-415
List_of_stars_in_Scorpius
Neutron star in the constellation Sagittarius
X-ray pulsations have been seen from SAX J1808.4-3658, making it a Rosetta stone for interpretation of the timing behavior of low-mass X-ray binaries
SAX_J1808.4−3658
High-mass X-ray binary
Ritter, H.; Kolb, U. (26 May 2003). "Catalogue of cataclysmic binaries, low–mass X-ray binaries and related objects (Seventh edition)". Astronomy & Astrophysics
4U_1543−475
Two pulsars orbiting each other
orbital eccentricities of IMBPs are significantly larger than those of low mass binary pulsars (LMBPs). As of 2014, there are fewer than 20 known IMBPs. Examples
Binary_pulsar
Globular cluster located in the constellation Sagittarius
PSR J1823-3021A. This globular cluster also contains 4U 1820-30, a low-mass X-ray binary with an orbital period of only 11.5 minutes, consisting of a neutron
NGC_6624
Star in the constellation Aquila
Aquila X-1 (frequently abbreviated to Aql X-1) is a low-mass x-ray binary (LMXB) and the most luminous X-Ray source in the constellation Aquila. It was
Aquila_X-1
Substellar object
brown dwarf's "surface". Using NASA's Chandra X-ray Observatory, scientists have detected X-rays from a low-mass brown dwarf in a multiple star system. This
Brown_dwarf
X-ray binary in the constellation Ara
galactic low-mass X-ray binary (LMXB) source and black hole candidate that flares from time to time. From spectroscopic measurements, the mass of the black-hole
GX_339−4
Type of x-ray binary
star) and a low-mass main-sequence star (i.e. a star with a mass less than the Sun's mass). These objects show dramatic changes in their X-ray emission,
Soft_X-ray_transient
Binary star in the constellation Circinus
Circinus X-1 is an X-ray binary star system that includes a neutron star. Observation of Circinus X-1 in July 2007 revealed the presence of X-ray jets normally
Circinus_X-1
Binary star in the constellation Monoceros
Reynolds, 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
A0620-00
NASA space telescope launched in 1999
The Chandra X-ray Observatory (CXO), previously known as the Advanced X-ray Astrophysics Facility (AXAF), is a Flagship-class space telescope launched
Chandra_X-ray_Observatory
Galaxy containing the Solar System
that the distribution of gamma-ray sources resembles that of low-mass X-ray binaries, suggesting that these X-ray binaries are sending positrons (and electrons)
Milky_Way
hydrogen-burning main-sequence stars LMXB – (celestial object) low-mass x-ray binary, an X-ray-luminous binary star system in which one of the stars is a neutron
List_of_astronomy_acronyms
Constellation split into two non-contiguous parts
few X-ray binaries. One of these, GX 17+2, is a low-mass X-ray binary consisting of a neutron star and, as in all low-mass X-ray binaries, a low-mass star
Serpens
Stellar core remnant
satellite. Low-mass helium white dwarfs (mass < 0.20 M☉), often referred to as extremely low-mass white dwarfs (ELM WDs), are formed in binary systems.
White_dwarf
Spectroscopic technique
X-ray photoelectron spectroscopy (XPS) is a surface-sensitive quantitative spectroscopic technique that measures the very topmost 50–60 atoms, 5–10 nm
X-ray photoelectron spectroscopy
X-ray_photoelectron_spectroscopy
Multiple system in the constellation Cygnus
"Near-infrared Spectroscopy of Low-mass X-ray Binaries: Accretion Disk Contamination and Compact Object Mass Determination in V404 Cyg and Cen X-4". The Astrophysical
V404_Cygni
High-mass X-ray binary star system in the constellation of Scorpius
OAO 1657-415 is a high-mass X-ray binary (HMXB) located in the constellation of Scorpius, over 20,000 light years away. It is believed to be composed
OAO_1657-415
Millisecond pulsar in the constellation Sagitta
M. (January 26, 2023). "Neutron star mass estimates from gamma-ray eclipses in spider millisecond pulsar binaries". Nature Astronomy. 7 (4): 451–462. arXiv:2301
Black_Widow_pulsar
Star in the constellation Corona Australis
2003). "A Spectroscopic and Photometric Study of the Eclipsing Low-mass X-Ray Binary 2A 1822-371 (V691 Coronae Australis". The Astronomical Journal.
V691_Coronae_Australis
Empirical function in astronomy
1365-2966.2009.14425.x. Dabringhausen, Jörg; Kroupa, Pavel; Pflamm-Altenburg, Jan; Mieske, Steffen (2012-03-01). "Low-Mass X-Ray Binaries Indicate a Top-Heavy
Initial_mass_function
Type of x-ray source
scaled-up X-ray binary or accreting IMBH. M74: Possibly containing an intermediate-mass black hole, as observed by Chandra in 2005. M82 X-1: This is
Ultraluminous_X-ray_source
Constellation in the northern celestial hemisphere
1% of its diameter. Discovered in 1990, UW Coronae Borealis is a low-mass X-ray binary system composed of a star less massive than the Sun and a neutron
Corona_Borealis
Transient x-ray binary system
X-ray pulsations have been seen from SAX J1808.4-3658, making it a Rosetta stone for interpretation of the timing behavior of low-mass X-ray binaries
X-ray_transient
Binary system in the constellation Aquila
GRS 1915+105 or V1487 Aquilae is an X-ray binary star system containing a main sequence star and a black hole. Transfer of material from the star to the
GRS_1915+105
Binary system consisting of a white dwarf and a main sequence star or a brown dwarf
Ritter, H.; Kolb, U. (June 2003). "Catalogue of cataclysmic binaries, low-mass X-ray binaries and related objects (Seventh edition)". Astronomy & Astrophysics
Post-common-envelope_binary
Planet that is outside the Milky Way galaxy
orbiting the high-mass X-ray binary M51-ULS-1 in the Whirlpool Galaxy was announced. The planet was detected by eclipses of the X-ray source, which consists
Extragalactic_planet
Globular cluster in the constellation Pegasus
White NE; Angelini L (2001). "The discovery of a second luminous low-mass X-ray binary in the globular cluster M15". Astrophysical Journal Letters. 561
Messier_15
transiting planet XO-1b UW CrB UW 16h 05m 45.87s +25° 51′ 45.17″ 19.7 Low-mass X-ray binary Table legend: • Name = Proper name • B = Bayer designation •
List of stars in Corona Borealis
List_of_stars_in_Corona_Borealis
Physical phenomenon of stars
system is an X-ray binary. A study in 2012 found that more than 70% of all massive stars exchange mass with a companion which leads to a binary merger in
Stellar_mass_loss
Pulsar with a rotational period less than about 10 milliseconds
Millisecond pulsars are thought to be related to low-mass X-ray binary systems. It is thought that the X-rays in these systems are emitted by the accretion disk
Millisecond_pulsar
Brown dwarf in the constellation Chamaleon
interpreted as strong variability of the x-ray emissions by this system. SDSS J1416+1348 UScoCTIO 108 Oph 162225-240515 Binary brown dwarfs W2150AB Brown, A. G
2MASS_J11011926−7732383
Star in the constellation Musca
Retrieved 8 December 2016. Liu, Q. Z. (2007). "A catalogue of low-mass X-ray binaries in the Galaxy, LMC, and SMC (Fourth edition)". Astronomy and Astrophysics
GRS_1124−683
1624-490 16h 28m 02.83s −49° 11′ 54.6″ Low-mass X-ray binary 4U 1630-47 16h 34m 01.61s −47° 23′ 34.8″ Low-mass X-ray binary Table legend: • Name = Proper name
List_of_stars_in_Norma
Astronomical objects colder than red dwarfs
can be either a low-mass star, a brown dwarf or a young free-floating planetary-mass object. If a young exoplanet or planetary-mass companion is detected
L_dwarf
Rapidly rotating x-ray binary system
orbital velocity. The star was the fastest moving star ever seen in an X-ray binary system until the discovery of system 47 Tuc X9. On the other hand, the
MAXI_J1659-152
X-ray source that only emits soft X-rays
luminous supersoft X-ray source (SSXS, or SSS) is an astronomical source that emits only low energy (i.e., soft) X-rays. Soft X-rays have energies in the
Supersoft_X-ray_source
X-ray Observatory have detected eleven X-ray sources, six of which were already known and five of which are new. Source A is a low-mass X-ray binary (LMXB)
NGC_6652
Compact astronomical body
to be a black hole. X-ray binaries can be categorised as either low-mass or high-mass; this classification is based on the mass of the companion star
Black_hole
Greek astrophysicist
gravitational waves, the emission of X-rays from compact binary objects and the coalescence of neutron-star binaries. Kalogera was born in 1971 in Serres
Vicky_Kalogera
Galaxy in the constellation Dorado
Chandra X-ray imaging of NGC 1553 show diffuse hot gas making up 70% of the emissions, dotted with many point-like sources (low-mass X-ray binaries) making
NGC_1553
Globular cluster in the constellation Tucana
completing a transition from being an accreting low-mass X-ray binary to a millisecond pulsar. X-ray emission has been individually detected from most
47_Tucanae
Flash of gamma rays from a distant galaxy
longer-lived afterglow is emitted, usually in the longer wavelengths of X-ray, ultraviolet, optical, infrared, microwave or radio frequencies. The intense
Gamma-ray_burst
Type of neutron star with beams of radiation
pulsars" (MSPs) had been found. MSPs are believed to be the end product of X-ray binaries. Owing to their extraordinarily rapid and stable rotation, MSPs can
Pulsar
Large self-illuminated object in space
The mass, radius, surface gravity, and rotation period can then be estimated based on stellar models. (Mass can be calculated for stars in binary systems
Star
travel, tourism, insurance
LOW MASS-X-RAY-BINARY
LOW MASS-X-RAY-BINARY
LOW MASS-X-RAY-BINARY
LOW MASS-X-RAY-BINARY
LOW MASS-X-RAY-BINARY
LOW MASS-X-RAY-BINARY
LOW MASS-X-RAY-BINARY
LOW MASS-X-RAY-BINARY
LOW MASS-X-RAY-BINARY
travel, tourism, insurance