Results 1 to 10 of about 1,969,668 (250)

Polarized x-rays constrain the disk-jet geometry in the black hole x-ray binary Cygnus X-1 [PDF]

open access: yesScience, 2022
A black hole x-ray binary (XRB) system forms when gas is stripped from a normal star and accretes onto a black hole, which heats the gas sufficiently to emit x-rays.
H. Krawczynski   +113 more
semanticscholar   +1 more source

Polarization Properties of the Weakly Magnetized Neutron Star X-Ray Binary GS 1826–238 in the High Soft State

open access: yesThe Astrophysical Journal, 2023
The launch of the Imaging X-ray Polarimetry Explorer (IXPE) on 2021 December 9 has opened a new window in X-ray astronomy. We report here the results of the first IXPE observation of a weakly magnetized neutron star, GS 1826−238, performed on 2022 March ...
Fiamma Capitanio   +96 more
doaj   +1 more source

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

The Metallicity Dependence of the High-mass X-Ray Binary Luminosity Function [PDF]

open access: yes, 2020
In this work, we present detailed constraints on the metallicity dependence of the high-mass X-ray binary (HMXB) X-ray luminosity function (XLF). We analyze ≈5 Ms of Chandra data for 55 actively star-forming galaxies at D ≲ 30 Mpc, with gas-phase ...
B. Lehmer   +9 more
semanticscholar   +1 more source

Be/X-ray binaries [PDF]

open access: yesAstrophysics and Space Science, 2011
"The final publication is available at http://www.springerlink.com".
Pablo Reig, Pablo Reig
openaire   +3 more sources

A radio parallax to the black hole X-ray binary MAXI J1820+070 [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society: Letters, 2019
Using the Very Long Baseline Array and the European Very Long Baseline Interferometry Network, we have made a precise measurement of the radio parallax of the black hole X-ray binary MAXI J1820+070, providing a model-independent distance to the source.
P. Atri   +23 more
semanticscholar   +1 more source

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

X-Ray Binary Luminosity Function Scaling Relations for Local Galaxies Based on Subgalactic Modeling [PDF]

open access: yesAstrophysical Journal Supplement Series, 2019
We present new Chandra constraints on the X-ray luminosity functions (XLFs) of X-ray binary (XRB) populations, as well as their scaling relations, for a sample of 38 nearby galaxies (D = 3.4–29 Mpc).
B. Lehmer   +9 more
semanticscholar   +1 more source

Clumpy Wind Studies and the Nondetection of a Cyclotron Line in OAO 1657–415

open access: yesThe Astrophysical Journal, 2023
Winds of massive stars are suspected to be inhomogeneous (or clumpy), which biases the measures of their mass-loss rates. In high-mass X-ray binaries (HMXBs), the compact object can be used as an orbiting X-ray point source to probe the wind and ...
Pragati Pradhan   +13 more
doaj   +1 more source

Discovery of a 2.8 s Pulsar in a 2 Day Orbit High-mass X-Ray Binary Powering the Ultraluminous X-Ray Source ULX-7 in M51 [PDF]

open access: yesAstrophysical Journal, 2019
We discovered 2.8 s pulsations in the X-ray emission of the ultraluminous X-ray source (ULX) M51 ULX-7 within the UNSEeN project, which was designed to hunt for new pulsating ULXs (PULXs) with XMM-Newton.
G. A. R. Castillo   +28 more
semanticscholar   +1 more source

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