Zobrazeno 1 - 8
of 8
pro vyhledávání: '"Dorota Gondek-Rosińska"'
Autor:
Mateusz Wiśniewicz, Dorota Gondek-Rosińska, Agnieszka Słowikowska, Andrzej Zdziarski, Agnieszka Janiuk
Publikováno v:
The Astrophysical Journal, Vol 944, Iss 2, p 214 (2023)
We present the results of the low-mass X-ray binary 4U 1636–536 study. We performed a temporal analysis of all available RXTE/All-Sky Monitor, RXTE/Proportional Counter Array, Swift/Burst Alert Telescope, and MAXI data collected until the middle of
Externí odkaz:
https://doaj.org/article/a04a4898d45e4fb3831fa30245116349
Publikováno v:
Proceedings of the International Astronomical Union. 16:350-351
Differential rotation in neutron stars allows for significantly larger masses than rigid rotation. Some of those hypermassive objects are, however, unstable and collapse to a black hole immediately after formation. Yet, the exact threshold of dynamic
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d996c1224d7ef8ab0ecb0fc1d818be56
https://doi.org/10.1017/s1743921322000977
https://doi.org/10.1017/s1743921322000977
Publikováno v:
Astrophys.J.
Astrophys.J., 2017, 837 (1), pp.58. ⟨10.3847/1538-4357/aa56c1⟩
Astrophys.J., 2017, 837 (1), pp.58. 〈10.3847/1538-4357/aa56c1〉
Astrophys.J., 2017, 837 (1), pp.58. ⟨10.3847/1538-4357/aa56c1⟩
Astrophys.J., 2017, 837 (1), pp.58. 〈10.3847/1538-4357/aa56c1〉
We study the main astrophysical properties of differentially rotating neutron stars described as stationary and axisymmetric configurations of a moderately stiff $\Gamma=2$ polytropic fluid. The high level of accuracy and of stability of our relativi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d0ec0d5e44fef2941472dbb13f75fd55
The current gravitational wave detectors have reached their operational sensitivity and are nearing detection of compact object binaries. In the coming years, we expect that the Advanced LIGO/VIRGO will start taking data. At the same time, there are
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ba8448a013ffd7a701bf167e8abbd053
A highly accurate, multi-domain spectral code is used in order to construct sequences of general relativistic, differentially rotating neutron stars in axisymmetry and stationarity. For bodies with a spheroidal topology and a homogeneous or an N=1 po
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::38c5a201dec2cbb0180612d8391d1dd1
Publikováno v:
Physical Review D
Physical Review D, American Physical Society, 2005, 71, pp.064012. ⟨10.1103/PhysRevD.71.064012⟩
Physical Review D, American Physical Society, 2005, 71, pp.064012. ⟨10.1103/PhysRevD.71.064012⟩
We present the first relativistic calculations of the final phase of inspiral of a binary system consisting of two stars built predominantely of strange quark matter (strange quark stars). We study the precoalescing stage within the Isenberg-Wilson-M
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::62c8dcfd3b28041aba6cac40632cadbc
We perform some numerical study of the secular triaxial instability of rigidly rotating homogeneous fluid bodies in general relativity. In the Newtonian limit, this instability arises at the bifurcation point between the Maclaurin and Jacobi sequence
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::510feccc15df31f2e041e7d00121c33b
Publikováno v:
Astrophysical Journal; 7/1/2019, Vol. 879 Issue 1, p1-1, 1p