Results 101 to 110 of about 12,989 (225)

INTEGRAL IBIS Catalog of Magnetar Bursts

open access: yesThe Astrophysical Journal
One of the distinctive properties of magnetars, young neutron stars powered mainly by magnetic energy, is the emission of short (≲1 s) bursts of hard X-rays. Such bursts have been observed in nearly all the known magnetars, although at different and time-
Dominik Patryk Pacholski   +2 more
doaj   +1 more source

Physics of Neutron Star Crusts

open access: yesLiving Reviews in Relativity, 2008
The physics of neutron star crusts is vast, involving many different research fields, from nuclear and condensed matter physics to general relativity.
Chamel Nicolas, Haensel Pawel
doaj  

Hydrogen-poor Superluminous Supernovae with Bumpy Light Curves Powered by Precessing Magnetars

open access: yesThe Astrophysical Journal
Recent observations and statistical studies have revealed that a significant fraction of hydrogen-poor superluminous supernovae (SLSNe-I) exhibit light curves that deviate from the smooth evolution predicted by the magnetar-powered model, instead showing
Biao Zhang   +3 more
doaj   +1 more source

Discovery of a radio emitting neutron star with an ultra-long spin period of 76 seconds. [PDF]

open access: yesNat Astron, 2022
Caleb M   +21 more
europepmc   +1 more source

Magnetar signature – the U curve [PDF]

open access: green, 2018
Vikram Soni   +4 more
openalex   +1 more source

A Target Search for Fast Radio Bursts Associated with Two Fast Blue Optical Transients: AT2018cow and CSS161010

open access: yesThe Astrophysical Journal
Fast blue optical transients (FBOTs) are luminous, rapidly evolving events with blue spectra, possibly powered by newborn magnetars and linked to fast radio bursts (FRBs).
Shi-Jie Gao   +7 more
doaj   +1 more source

Born–Infeld magnetars: larger than classical toroidal magnetic fields and implications for gravitational-wave astronomy

open access: yesEuropean Physical Journal C: Particles and Fields, 2018
Magnetars are neutron stars presenting bursts and outbursts of X- and soft-gamma rays that can be understood with the presence of very large magnetic fields.
Jonas P. Pereira   +2 more
doaj   +1 more source

A giant glitch from the magnetar SGR J1935+2154 before FRB 200428 [PDF]

open access: green, 2022
Mingyu Ge   +13 more
openalex   +1 more source

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