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Published in 2020 at "Astronomy and Astrophysics"
DOI: 10.1051/0004-6361/202038791
Abstract: Context. In high mass X-ray binaries, an accreting compact object orbits a high mass star which loses mass through a dense and
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Keywords:
radiography high;
mass;
mass ray;
ray binaries ... See more keywords
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Published in 2021 at "Astronomy and Astrophysics"
DOI: 10.1051/0004-6361/202039785
Abstract: The soft gamma-ray repeater candidate SGR 0755$-$2933 was discovered in 2016 by Swift/BAT, which detected a short ($\sim$30 ms) powerful burst typical of magnetars. To understand the nature of the source, we present here an…
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Keywords:
new high;
sgr 0755;
mass ray;
0755 2933 ... See more keywords
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Published in 2021 at "Astronomy and Astrophysics"
DOI: 10.1051/0004-6361/202140545
Abstract: The final aim of this paper is to expand the sparse group of X-ray binaries with gamma-ray counterparts as laboratories to study high-energy processes under physical conditions that periodically repeat. A follow-up of a candidate…
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Keywords:
period;
orbital period;
mass ray;
ray ... See more keywords
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Published in 2021 at "Research in Astronomy and Astrophysics"
DOI: 10.1088/1674-4527/ac3125
Abstract: Using the apparent correlation of luminosity (LX) versus displacement (R) of high mass X-ray binaries (HMXBs), we aim to constrain the common envelope (CE) mechanism, which is vital in the formation and evolution of compact…
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Keywords:
luminosity versus;
versus displacement;
correlation;
mass ray ... See more keywords
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Published in 2020 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/staa675
Abstract: The application of standard accretion theory to observations of X-ray binaries provides valuable insights into neutron star properties, such as their spin period and magnetic field. However, most studies concentrate on relatively old systems, where…
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Keywords:
neutron star;
mass ray;
high mass;
ray binaries ... See more keywords
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Published in 2021 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/stab2231
Abstract: We report a detailed modelling of soft X-ray emission lines from two stellar wind-fed Galactic high-mass X-ray binary (HMXB) systems, Cyg X-3 and 4U 1538-522, and estimate physical parameters, e.g. hydrogen density, radiation field, chemical…
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Keywords:
field;
mass ray;
cyg 1538;
high mass ... See more keywords
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Published in 2017 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/stw2961
Abstract: We analyse all available RXTE data on a sample of 13 low-mass X-ray binaries with known neutron star spin that are not persistent pulsars. We carefully measure the correlations between the centroid frequencies of the…
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Keywords:
frequency;
neutron star;
mass ray;
precession ... See more keywords
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Published in 2017 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/stx671
Abstract: We present 3–79 keV NuSTAR observations of the neutron star low-mass X-ray binary 4U 1636−53 in the soft, transitional and hard state. The spectra display a broad emission line at 5–10 keV. We applied several…
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Keywords:
line;
mass ray;
binary 1636;
low mass ... See more keywords
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Published in 2018 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/sty1612
Abstract: We have identified 55 candidate high-mass X-ray binaries (HMXBs) in M33 using available archival {\it HST} and {\it Chandra} imaging to find blue stars associated with X-ray positions. We use the {\it HST} photometric data…
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Keywords:
mass;
formation;
mass ray;
ray binaries ... See more keywords
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Published in 2019 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/stz2929
Abstract: The heating of the intergalactic medium in the early, metal-poor Universe may have been partly due to radiation from high-mass X-ray binaries (HMXBs). Previous investigations on the effect of metallicity have used galaxies of different…
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Keywords:
effects metallicity;
mass ray;
metallicity;
ray ... See more keywords
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Published in 2019 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/stz3082
Abstract: The orbital profile of the high-mass X-ray binary IGR J16393−4643 shows a dip in its X-ray intensity, which was previously interpreted as an eclipse. Unlike most eclipsing HMXBs, where the X-ray eclipses are about two…
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Keywords:
intensity;
ray binary;
mass ray;
ray ... See more keywords