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High Mass X-ray Binaries : the donor stars and their compact companions [PDF]
, 2008 This thesis presents new spectroscopic observations of the donor star in several High Mass X-ray Binary systems. The various types of X-ray Binary systems that exist are outlined and the methods and limitations of mass determination of the stellar components are discussed. The masses of the compact objects are determined for the systems SMC X-1 and LMC
Amira Val Baker
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A high-mass X-ray binary descended from an ultra-stripped supernova
Nature, 2023Ultra-stripped supernovae are different from other terminal explosions of massive stars, as they show little or no ejecta from the actual supernova event^ 1 , 2 .
N. Richardson +8 more
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Common origin for black holes in both high mass X-ray binaries and gravitational-wave sources
Astronomy & Astrophysics, 2021Black-hole (BH) high-mass X-ray binary (HMXB) systems are likely to be the progenitors of BH-BH mergers detected in gravitational waves by LIGO/Virgo/KAGRA (LVK).
K. Belczynski +4 more
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Investigation of the Disk of the Be Star in the High-Mass X-ray Binary IGR J21343+4738
Письма в Астрономический журнал: Астрономия и космическая астрофизика, 2023We present the results of our long-term photometric and spectroscopic monitoring with the1.5-m telescope RTT-150 for the optical counterpart of the high-mass X-ray binary IGR J21343+4738discovered in 2002 by the INTEGRAL space X-ray observatory. The X-ray source was also repeatedlydetected by the telescopes of the SRG observatory during the all-sky ...
E. A. Nikolaeva +6 more
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Evolution of High-mass X-ray binaries in the Small Magellanic Cloud
Proceedings of the International Astronomical Union, 2018In order to understand the progenitor of rotation powered pulsars, we compare them with High-mass X-ray binary (HMXB) pulsars, (or X-ray pulsars), in the Small Magellanic Cloud. The plot of period period vs.
Jun Yang, D. Wik
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Accreting Neutron Stars in Low-Mass X-Ray Binary Systems
, 2007Using the Rossi X-ray Timing Explorer (RossiXTE ), astronomers have discovered that disk-accreting neutron stars with weak magnetic fields produce three distinct types of high-frequency X-ray oscillations. These oscillations are powered by release of the
F. Lamb, S. Boutloukos
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Monitoring Neutron Star High-Mass X-Ray Binaries in the INTEGRAL Galactic Plane Survey
AIP Conference Proceedings, 2006Monitoring neutron star systems allows to measure the flux and pulse period evolution of these systems, which in turn helps in studying their accretion history and the physics of the interaction between the accretion disk and the neutron star’s magnetic field. This contribution presents information on the ongoing monitoring activities with the INTEGRAL
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2012
My thesis centers around the study of neutron stars, especially those in massive binary systems. To this end, it has two distinct components: the observational study of neutron stars in massive binaries with a goal of measuring neutron star masses and participation in NuSTAR, the first imaging hard X-ray mission, one that is extremely well suited to ...
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My thesis centers around the study of neutron stars, especially those in massive binary systems. To this end, it has two distinct components: the observational study of neutron stars in massive binaries with a goal of measuring neutron star masses and participation in NuSTAR, the first imaging hard X-ray mission, one that is extremely well suited to ...
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Massive Stars and Their Compact Remnants in High-Mass X-Ray Binaries
, 2007 L. Kaper, A. van der Meer
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