Zobrazeno 1 - 10
of 21
pro vyhledávání: '"Jared Rice"'
Publikováno v:
The Astrophysical Journal, Vol 963, Iss 2, p 156 (2024)
The nearby long-duration GRB 191019A recently detected by Swift lacks an associated supernova and belongs to a host galaxy with little star formation activity, suggesting that the origin of this burst is the result of a merger of two compact objects
Externí odkaz:
https://doaj.org/article/58cae327423f4b939c6069325d809b71
Autor:
Hou-Jun Lü, Hao-Yu Yuan, Ting-Feng Yi, Xiang-Gao Wang, You-Dong Hu, Yong Yuan, Jared Rice, Jian-Guo Wang, Jia-Xin Cao, De-Feng Kong, Emilio Fernandez-García, Alberto J. Castro-Tirado, Ji-Shun Lian, Wen-Pei Gan, Shan-Qin Wang, Li-Ping Xin, M. D. Caballero-García, Yu-Feng Fan, En-Wei Liang
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
This is an Open Access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the origina
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::dc7417c70283900379861b743ebee600
http://hdl.handle.net/10261/278869
http://hdl.handle.net/10261/278869
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 492:3622-3630
Short gamma-ray bursts (GRB) with extended emission (EE) that are composed of an initial short hard spike followed by a long-lasting EE are thought to comprise a sucategory of short GRBs. The narrow energy band available during the Swift era, combine
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::28f7935d604fe9f9efd0c099e7bae1dc
https://doi.org/10.1093/mnras/staa044
https://doi.org/10.1093/mnras/staa044
The growing observed evidence shows that the long- and short-duration gamma-ray bursts (GRBs) originate from massive star core-collapse and the merger of compact stars, respectively. GRB 201221D is a short-duration GRB lasting $\sim 0.1$ s without ex
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::da8dc614de522f90df90bf92dd60729d
Weak and continuous gravitational-wave (GW) radiation can be produced by newborn magnetars with deformed structure and is expected to be detected by the Einstein telescope in the near future. In this work we assume that the deformed structure of a na
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bae0e7b180f63a67e55bf86be9c8ef45
We used archival data from the \emph{Chandra X-ray Observatory} (\emph{Chandra}) and the \emph{Hubble Space Telescope}, to identify 334 candidate X-ray binary (XRB) systems and their potential optical counterparts in the interacting galaxy pair NGC 5
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::52b7ccf9490fb0331e74255b326c958b
Observationally, there is a small fraction of Gamma-ray bursts (GRBs) with prompt emission observed by Fermi/GBM that are composed of two pulses. Occasionally, the distance to a GRB may be lensed when a high mass astrophysical object resides in the p
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8e1bd5620ca345e6017c36987d157901
The observed internal plateau of X-ray emission in some short GRBs suggests the formation of a remnant supra-massive magnetar following a double neutron star (NS) merger. In this paper, we assume that the rotational energy is lost mainly via gravitat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::17c3987f4e97f51c62ccd07e9ecd6ee1
http://arxiv.org/abs/2001.05355
http://arxiv.org/abs/2001.05355
The event GW170817/GRB 170817A, discovered via the successful joint observation of its gravitational wave radiation and its multi-wavelength electromagnetic counterparts, was the first definite "smoking-gun" from the merger of two neutron stars (NSs)
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::454f5762dd68a52f977e8e743a98a461
Autor:
Jared Rice, Bing Zhang
Publikováno v:
The Astrophysical Journal. 908:59
A stellar mass black hole can grow its mass noticeably through Bondi accretion, if it is embedded in an extremely dense and massive molecular cloud with slow motion with respect to the ambient medium for an extended period of time. This provides a no
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::92b883835311003b8c6b4b82ca063615
https://doi.org/10.3847/1538-4357/abd6ea
https://doi.org/10.3847/1538-4357/abd6ea