Results 11 to 20 of about 130,686 (336)

Magnetic Inclination Evolution of Accreting Neutron Stars in Intermediate/Low-mass X-Ray Binaries [PDF]

open access: yesThe Astrophysical Journal, 2023
The magnetic inclination angle χ , namely the angle between the spin and magnetic axes of a neutron star, plays a vital role in its observational characteristics. However, there are few systematic investigations of its long-term evolution, especially for
Hao-ran Yang, Xiang-dong Li
doaj   +2 more sources

Discovery of strongly variable X-ray polarization in the neutron star low-mass X-ray binary transient XTE J1701−462 [PDF]

open access: yesAstronomy & Astrophysics, 2023
After about 16 years since its first outburst, the transient neutron star low-mass X-ray binary XTE J1701$-$462 turned on again in September 2022, allowing for the first study of its X-ray polarimetric characteristics by a dedicated observing program ...
M. Cocchi   +107 more
semanticscholar   +1 more source

Investigating the Lower Mass Gap with Low-mass X-Ray Binary Population Synthesis [PDF]

open access: yesAstrophysical Journal, 2022
Mass measurements from low-mass black hole X-ray binaries (LMXBs) and radio pulsars have been used to identify a gap between the most massive neutron stars (NSs) and the least massive black holes (BHs).
Jared C. Siegel   +16 more
semanticscholar   +1 more source

Magnetic Braking with MESA Evolutionary Models in the Single Star and Low-mass X-Ray Binary Regimes [PDF]

open access: yesAstrophysical Journal, 2022
Magnetic braking has a prominent role in driving the evolution of close low-mass binary systems and heavily influences the rotation rates of low-mass F- and later-type stars with convective envelopes. Several possible prescriptions that describe magnetic
S. Gossage, V. Kalogera, Meng Sun
semanticscholar   +1 more source

Constraining the properties of dense neutron star cores: The case of the low-mass X-ray binary HETE J1900.1–2455 [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2021
Measuring the time evolution of the effective surface temperature of neutron stars can provide invaluable information on the properties of their dense cores.
N. Degenaar   +5 more
semanticscholar   +1 more source

The Equation of State and Some Key Parameters of Neutron Stars: Constraints from GW170817, the Nuclear Data, and the Low-mass X-Ray Binary Data [PDF]

open access: yesAstrophysical Journal, 2019
In this work we parameterize the equation of state of dense neutron star (NS) matter with four pressure parameters of and then set the combined constraints with the data of GW170817 and the data of six low-mass X-ray binaries (LMXBs) with thermonuclear ...
Jin-Liang Jiang   +8 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

PSR J1953+1844 Probably Being the Descendant of an Ultracompact X-Ray Binary

open access: yesThe Astrophysical Journal Letters, 2023
PSR J1953+1844 (i.e., M71E) is a millisecond pulsar in a 53 minute binary orbit discovered by the Five-hundred-meter Aperture Spherical radio Telescope. The mass function from pulsar timing is 2.3 × 10 ^−7 M _⊙ .
Z. L. Yang   +3 more
doaj   +1 more source

Donors of Persistent Neutron-Star Low-Mass X-Ray Binaries [PDF]

open access: yesPublications of the Astronomical Society of the Pacific, 2012
Properties of X-ray luminosities in low-mass X-ray binaries (LMXBs) mainly depend on donors. We have carried out a detailed study of donors in persistent neutron-star LMXBs (PLMXBs) by means of a population synthesis code. PLMXBs with different donors have different formation channels.
Zhu, Chunhua   +3 more
openaire   +2 more sources

UPPER BOUNDS ON r-MODE AMPLITUDES FROM OBSERVATIONS OF LOW-MASS X-RAY BINARY NEUTRON STARS [PDF]

open access: yes, 2013
We present upper limits on the amplitude of r-mode oscillations and gravitational-radiation-induced spin-down rates in low-mass X-ray binary neutron stars, under the assumption that the quiescent neutron star luminosity is powered by dissipation from a ...
S. Mahmoodifar, T. Strohmayer
semanticscholar   +1 more source

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