Results 71 to 80 of about 142,213 (355)

The spatial correlation of high-mass X-ray binaries and young star clusters in nearby star-forming galaxies

open access: yesMonthly Notices of the Royal Astronomical Society, 2023
ABSTRACT We present an analysis of the two-point spatial correlation functions of high-mass X-ray binary (HMXB) and young star cluster (YSC) populations in M31 and M33. We find evidence that HMXBs are spatially correlated with YSCs to a higher degree than would be expected from random chance in both galaxies.
Breanna A Binder   +4 more
openaire   +2 more sources

Near-infrared spectroscopy of 20 new Chandra sources in the Norma Arm

open access: yes, 2014
We report on CTIO/NEWFIRM and CTIO/OSIRIS photometric and spectroscopic observations of 20 new X-ray (0.5-10 keV) emitters discovered in the Norma Arm Region Chandra Survey (NARCS).
Bauer, Franz E.   +4 more
core   +1 more source

Multi-wavelength observations of Galactic hard X-ray sources discovered by INTEGRAL. I. The nature of the companion star [PDF]

open access: yes, 2008
Context: The INTEGRAL hard X-ray observatory has revealed an emerging population of highly obscured X-ray binary systems through multi-wavelength observations.
Bird   +80 more
core   +5 more sources

Neutron Stars in X-ray Binaries and their Environments

open access: yes, 2017
Neutron stars in X-ray binary systems are fascinating objects that display a wide range of timing and spectral phenomena in the X-rays. Not only parameters of the neutron stars, like magnetic field strength and spin period evolve in their active binary ...
Paul, Biswajit
core   +1 more source

Formation of wind-fed black hole high-mass X-ray binaries: The role of Roche-lobe-overflow post black hole formation [PDF]

open access: yesAstronomy & Astrophysics
The three dynamically confirmed wind-fed black hole high-mass X-ray binaries (BH-HMXBs) are suggested to all contain a highly spinning black hole (BH).
Zepei Xing   +14 more
semanticscholar   +1 more source

Formation of Sco X-1 induced by anomalous magnetic braking of Ap/Bp stars

open access: yes, 2017
Sco X-1 is the brightest persistent X-ray in the sky. It is generally believed that Sco X-1 is a low-mass X-ray binary containing a neutron star accreting from a low-mass donor star where mass transfer is driven by the magnetic braking. However, the mass
Chen, Wen-Cong
core   +1 more source

A new model for the X-ray continuum of the magnetized accreting pulsars [PDF]

open access: yes, 2016
Accreting highly magnetized pulsars in binary systems are among the brightest X-ray emitters in our Galaxy. Although a number of high statistical quality broad-band (0.1-100 keV) X-ray observations are available, the spectral energy distribution of these
Becker, P. A.   +3 more
core   +2 more sources

Three New Galactic Center X-ray Sources Identified with Near-Infrared Spectroscopy

open access: yes, 2013
We have conducted a near-infrared spectroscopic survey of 47 candidate counterparts to X-ray sources discovered by the Chandra X-ray Observatory near the Galactic Center (GC).
Bandyopadhyay, Reba M.   +7 more
core   +1 more source

An Overabundance of Transient X-ray Binaries within 1 pc of the Galactic Center

open access: yes, 2004
During five years of Chandra observations, we have identified seven X-ray transients located within 23 pc of Sgr A*. These sources each vary in luminosity by more than a factor of 10, and have peak X-ray luminosities greater than 5e33 erg/s, which ...
A. Ghez   +10 more
core   +1 more source

The origin of Scorpius X-1 [PDF]

open access: yes, 2003
We have used multi-wavelength observations of high precision to derive the space velocity and compute the orbit around the Galactic Centre of the prototype X-ray binary Scorpius X-1. An origin in the local spiral arm of the Milky Way is ruled out.
Mirabel, I. Felix, Rodrigues, Irapuan
core   +3 more sources

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