A state change in the low-mass X-ray binary XSS J12270− 4859
CG Bassa, A Patruno, JWT Hessels… - Monthly Notices of …, 2014 - academic.oup.com
Millisecond radio pulsars acquire their rapid rotation rates through mass and angular
momentum transfer in a low-mass X-ray binary system. Recent studies of PSR J1824− 2452I …
momentum transfer in a low-mass X-ray binary system. Recent studies of PSR J1824− 2452I …
[HTML][HTML] Science with e-ASTROGAM: A space mission for MeV–GeV gamma-ray astrophysics
A De Angelis, V Tatischeff, IA Grenier, J McEnery… - Journal of High Energy …, 2018 - Elsevier
Abstract e-ASTROGAM ('enhanced ASTROGAM') is a breakthrough Observatory space
mission, with a detector composed by a Silicon tracker, a calorimeter, and an …
mission, with a detector composed by a Silicon tracker, a calorimeter, and an …
Accreting pulsars: mixing-up accretion phases in transitional systems
S Campana, TD Salvo - The Physics and Astrophysics of Neutron Stars, 2018 - Springer
In the last 20 years our understanding of the millisecond pulsar population changed
dramatically. Thanks to the large effective area and good time resolution of the NASA X-ray …
dramatically. Thanks to the large effective area and good time resolution of the NASA X-ray …
The second catalog of flaring gamma-ray sources from the Fermi All-sky Variability Analysis
S Abdollahi, M Ackermann, M Ajello… - The Astrophysical …, 2017 - iopscience.iop.org
We present the second catalog of flaring gamma-ray sources (2FAV) detected with the Fermi
All-sky Variability Analysis (FAVA), a tool that blindly searches for transients over the entire …
All-sky Variability Analysis (FAVA), a tool that blindly searches for transients over the entire …
Optical pulsations from a transitional millisecond pulsar
F Ambrosino, A Papitto, L Stella, F Meddi, P Cretaro… - Nature …, 2017 - nature.com
Millisecond pulsars are neutron stars that attain their very fast rotation during a 108–109-yr-
long phase of disk accretion of matter from a low-mass companion star,. They can be …
long phase of disk accretion of matter from a low-mass companion star,. They can be …
Discovery of PSR J1227− 4853: A transition from a low-mass X-ray binary to a redback millisecond pulsar
J Roy, PS Ray, B Bhattacharyya… - The Astrophysical …, 2015 - iopscience.iop.org
ABSTRACT XSS J12270− 4859 is an X-ray binary associated with the Fermi Large Area
Telescope gamma-ray source 1FGL J1227. 9− 4852. In 2012 December, this source …
Telescope gamma-ray source 1FGL J1227. 9− 4852. In 2012 December, this source …
Coordinated X-ray, ultraviolet, optical, and radio observations of the PSR J1023+ 0038 system in a low-mass X-ray binary state
S Bogdanov, AM Archibald, C Bassa… - The Astrophysical …, 2015 - iopscience.iop.org
The PSR J1023+ 0038 binary system hosts a neutron star and a low-mass, main-sequence-
like star. It switches on year timescales between states as an eclipsing radio millisecond …
like star. It switches on year timescales between states as an eclipsing radio millisecond …
Transitional millisecond pulsars
A Papitto, D Martino - Millisecond Pulsars, 2021 - Springer
Millisecond pulsars in tight binaries have recently challenged our understanding of physical
processes governing the evolution of binaries and the interaction between astrophysical …
processes governing the evolution of binaries and the interaction between astrophysical …
X-ray states of redback millisecond pulsars
M Linares - The Astrophysical Journal, 2014 - iopscience.iop.org
Compact binary millisecond pulsars with main-sequence donors, often referred to as"
redbacks," constitute the long-sought link between low-mass X-ray binaries and millisecond …
redbacks," constitute the long-sought link between low-mass X-ray binaries and millisecond …