Results 11 to 20 of about 142,213 (355)
Evolution of neutron stars in high-mass X-ray binaries [PDF]
Monthly Notices of the Royal Astronomical Society, 1998 We consider the evolution of neutron stars during the X-ray phase of high-mass binaries. Calculationsareperformedassumingacrustal originofthemagneticfield.Astrongwindfrom the companion can significantly influence the magnetic and spin behaviour of a neutron star even during the main-sequence life of the companion.
V. Urpin, D. Konenkov, U. Geppert
semanticscholar +3 more sources
The High Mass X-ray binaries in star-forming galaxies [PDF]
Proceedings of the International Astronomical Union, 2018 The high mass X-ray binaries (HMXBs) provide an exciting framework to investigate the evolution of massive stars and the processes behind binary evolution.
M. Celeste Artale +3 more
semanticscholar +4 more sources
High-mass X-ray Binaries and OB-runaway Stars [PDF]
, 2001 High-mass X-ray binaries (HMXBs) represent an important phase in the evolution of massive binary systems. HMXBs provide unique diagnostics to test massive-star evolution, to probe the physics of radiation-driven winds, to study the process of mass accretion, and to measure fundamental parameters of compact objects.
L. Kaper
openalex +5 more sources
Tidal Interaction in High Mass X-ray Binaries and Symbiotic Stars [PDF]
, 2010 9 pages, to appear in Bulgarian Astron ...
R. Zamanov
openalex +3 more sources
Feeding Neutron Stars in High-Mass X-ray Binaries [PDF]
Proceedings of the International Astronomical Union, 2012 AbstractWe suggest that the Be/X-ray binary SXP 1062 and the supergiant fast X-ray transient AX J1841.0-0536 belong to accreting magnetars and anti-magnetars, respectively.
Lei Fu, Zidong Zhang, Xiang‐Dong Li
openalex +2 more sources
A New Class of High-Mass X-Ray Binaries: Implications for Core Collapse and Neutron Star Recoil [PDF]
The Astrophysical Journal, 2001 We investigate an interesting new class of high-mass X-ray binaries (HMXBs) with long orbital periods (Porb > 30 days) and low eccentricities (e ≲ 0.2).
E. Pfahl +3 more
semanticscholar +7 more sources
Massive Stars and their Compact Remnants in High-mass X-ray Binaries [PDF]
, 2005 In a high-mass X-ray binary (HMXB) a massive star interacts with a neutron-star or black-hole companion in various ways. The gravitational interaction enables the measurement of fundamental parameters such as the mass of both binary components, providing important constraints on the evolutionary history of the system, the equation of state of matter at
L. Kaper, A. van der Meer
openalex +4 more sources
High-Mass X-Ray Binaries and OB Runaway Stars [PDF]
International Astronomical Union Colloquium, 2004 AbstractHigh-mass X-ray binaries (HMXBs) represent an important phase in the evolution of massive binary systems and provide fundamental information on the properties of the OB-star primaries and their compact secondaries (neutron star, black hole). Recent observations indicate that the neutron stars in some of these systems (Vela X-1, 4U 1700-37) are ...
L. Kaper, A. van der Meer, A. Tijani
openalex +3 more sources
MASSES OF NEUTRON STARS IN HIGH-MASS X-RAY BINARIES WITH OPTICAL ASTROMETRY [PDF]
The Astrophysical Journal, 2010 Determining the type of matter that is inside a neutron star (NS) has been a long-standing goal of astrophysics. Despite this, most of the NS equations of state (EOS) that predict maximum masses in the range 1.4-2.8 solar masses are still viable. Most of the precise NS mass measurements that have been made to date show values close to 1.4 solar masses,
John A. Tomsick, Matthew W. Muterspaugh
openalex +4 more sources
Exploration of spin-down rate of neutron stars in high-mass X-ray binaries [PDF]
Monthly Notices of the Royal Astronomical Society, 2016 We use the evolutionary population synthesis method to investigate the statistical properties of the wind-fed neutron star (NS) compact ($P_{\rm orb}<10$ days) high-mass X-ray binaries (HMXBs) in our Galaxy, based on different spin-down models. We find that the spin-down rate in the supersonic propeller phase given \textbf{by assuming that the ...
Hai‐Lang Dai +2 more
openalex +3 more sources