Results 1 to 10 of about 130,686 (336)

Accreting Neutron Stars in Low-Mass X-Ray Binary Systems [PDF]

open access: yes, 2007
Using 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.
A Cumming   +90 more
core   +3 more sources

Rapid X-Ray Variability of Neutron Stars in Low-Mass Binary Systems [PDF]

open access: yesNuclear Physics B - Proceedings Supplements, 1998
The dramatic discovery with the Rossi X-Ray Timing Explorer satellite of remarkably coherent $\sim$300--1200 Hz oscillations in the X-ray brightness of some sixteen neutron stars in low-mass binary systems has spurred theoretical modeling of these ...
Alpar   +41 more
core   +4 more sources

News on the X-ray emission from hot subdwarf stars [PDF]

open access: yesOpen Astronomy, 2017
In latest years, the high sensitivity of the instruments on-board the XMM-Newton and Chandra satellites allowed us to explore the properties of the X-ray emission from hot subdwarf stars.
Palombara Nicola La, Mereghetti Sandro
doaj   +3 more sources

X-Ray Polarization Study of the Neutron Star Low-mass X-Ray Binary GX 349+2

open access: yesThe Astrophysical Journal
We report the first X-ray polarimetric results of the neutron star (NS) low-mass X-ray binary Z-source GX 349+2 using the Imaging X-ray Polarimetry Explorer (IXPE). We discovered that the X-ray source was polarized at a polarization degree of PD = 1.1% ± 
Unnati Kashyap   +5 more
doaj   +3 more sources

X-Ray and Radio Polarimetry of the Neutron Star Low-mass X-Ray Binary GX 13+1

open access: yesThe Astrophysical Journal
We report the X-ray and radio polarization study of the neutron star low-mass X-ray binary (LMXB) GX 13+1 using the Imaging X-ray Polarimetry Explorer (IXPE) and Very Large Array.
Unnati Kashyap   +5 more
doaj   +3 more sources

X-Ray and Radio Polarimetry of the Neutron Star Low-mass X-Ray Binary 4U 1728–34

open access: yesThe Astrophysical Journal
We report the first X-ray and radio polarimetric results of the neutron star (NS) low-mass X-raydis binary atoll-source 4U 1728−34 using the Imaging X-ray Polarimetry Explorer (IXPE) and Australia Telescope Compact Array.
Unnati Kashyap   +6 more
doaj   +3 more sources

Search for intermittent X-ray pulsations from neutron stars in low-mass X-ray binaries [PDF]

open access: yesPublications of the Astronomical Society of Australia, 2021
AbstractWe present the results of our extensive binary orbital motion corrected pulsation search for 13 low-mass X-ray binaries. These selected sources exhibit burst oscillations in X-rays with frequencies ranging from 45 to 1 122 Hz and have a binary orbital period varying from 2.1 to 18.9 h.
Yunus Emre Bahar   +2 more
openaire   +4 more sources

Spectral Energy Distributions of Southern Binary X-Ray Sources

open access: yesThe Astrophysical Journal Supplement Series, 2023
The rapid variability of X-ray binaries (XRBs) produces a wide range of X-ray states that are linked to activity across the electromagnetic spectrum. It is particularly challenging to study a sample of sources large enough to include all types in their ...
John M. Dickey   +7 more
doaj   +1 more source

Low-Mass X-Ray Binaries with Strange Quark Stars [PDF]

open access: yesPublications of the Astronomical Society of the Pacific, 2013
Strange quark stars (SSs) may originate from accreting neutron stars (NSs) in low-mass X-ray binaries (LMXBs). Assuming that conversion of NS matter to SSs occurs when the core density of accreting NS reaches to the density of quark deconfinement, $\sim 5 _0$, where $ _0\sim 2.7\times 10^{14}$g cm$^{-3}$ is nuclear saturation density, we investigate
Zhu, Chunhua   +3 more
openaire   +2 more sources

An Optically Discovered Outburst from XTE J1859+226

open access: yesThe Astrophysical Journal, 2023
Using the Zwicky Transient Facility, in 2021 February we identified the first known outburst of the black hole X-ray transient XTE J1859+226 since its discovery in 1999. The outburst was visible at X-ray, UV, and optical wavelengths for less than 20 days,
Eric C. Bellm   +15 more
doaj   +1 more source

Home - About - Disclaimer - Privacy