Results 21 to 30 of about 85,552 (296)
Back to Business: SLX 1746–331 after 13 Years of Silence
The Astrophysical Journal, 2023 The black hole candidate system SLX 1746–331 was back to business in 2023, after a long silence of roughly 13 years. An outburst was observed thoroughly by Insight-HXMT and NICER.
Jing-Qiang Peng +19 more
doaj +1 more source
Magnetic Fields of Neutron Stars in X-Ray Binaries [PDF]
Space Science Reviews, 2014 16 pages, 9 figures, invited topical review, to be published in The Strongest Magnetic Fields in the Universe (Space Sciences Series of ISSI, Springer), Space Science Reviews ...
Revnivtsev, Mikhail, MEREGHETTI, Sandro
openaire +3 more sources
Accretion Onto the Neutron Star in Be/X-ray Binaries [PDF]
Symposium - International Astronomical Union, 2004 We study accretion onto the neutron star in Be/X-ray binaries, using a 3D SPH code and the data imported from a high resolution simulation by Okazaki et al. (2002) for a coplanar system with a short period (Porb = 24.3 d) and moderate eccentricity (e = 0.34).
Hayasaki, Kimitake, Okazaki, Atsuo. T.
openaire +2 more sources
X-Raying the Birth of Binary Neutron Stars and Neutron Star–Black Hole Binaries
The Astrophysical Journal, 2022 Abstract We consider fallback accretion after an ultrastripped supernova (USSN) that accompanies formation of a binary neutron star (BNS) or a neutron star–black hole binary (NS–BH). The fallback matter initially accretes directly to the nascent NS, while it starts to accrete to the circumbinary disk, typically 0.1–1 day after the onset ...
Kazumi Kashiyama, Ryo Sawada, Yudai Suwa
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Beam Pattern Evolution of Accreting X-Ray Pulsar 1A 0535+262 during Its 2020 Giant Outburst
The Astrophysical Journal, 2023 We report on pulse profile decomposition analysis of bright transient X-ray pulsar 1A 0535+262 using broadband Insight-HXMT observations during a giant outburst of the source in 2020.
Y. F. Hu +9 more
doaj +1 more source
Magnetic Flares on Asymptotic Giant Branch Stars [PDF]
, 2002 We investigate the consequences of magnetic flares on the surface of asymptotic giant branch (AGB) and similar stars. In contrast to the solar wind, in the winds of AGB stars the gas cooling time is much shorter than the outflow time.
Bochanski J. J. +13 more
core +4 more sources
Debris Disks around Solar-Type Stars: Observations of the Pleiades with Spitzer Space Telescope [PDF]
, 2010 We present Spitzer MIPS observations at 24 um of 37 solar-type stars in the Pleiades and combine them with previous observations to obtain a sample of 71 stars.
Gorlova, N. I. +5 more
core +2 more sources
Be stars in X-ray binary systems [PDF]
International Astronomical Union Colloquium, 2000 AbstractThis paper will review the status of our observations and understanding of Be stars in X-ray binary systems. In virtually all cases the binary partner to the Be star is a neutron star. The circumstellar disk provides the accretion fuel and hence stimulates the X-ray emission, whilst the neutron star provides a valuable probe of the environment ...
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Bowen Fluorescence from Companion Stars in X-Ray Binaries [PDF]
International Astronomical Union Colloquium, 2004 AbstractThis paper will review a new technique of detecting companion stars in LMXBs and X-ray transients in outburst using the Bowen fluorescence NIII lines at 4634-4640. These lines are very efficiently reprocessed in the atmospheres of the companion stars and, thereby, provide estimates of the K2 velocities and mass functions.
Casares, J +5 more
openaire +3 more sources
A CORAVEL radial-velocity monitoring of S stars: symbiotic activity vs. orbital separation [PDF]
, 1998 Orbital elements are presented for the Tc-poor S stars HR 363 (= HD 7351) and HD 191226. With an orbital period of 4592 d (=12.6 y), HR 363 has the longest period known among S stars, and yet it is a strong X-ray source. Its X-ray flux is similar to that
Carquillat, J. M. +3 more
core +1 more source