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Academic Articles & Research Papers
Showing 6 of 6 academic articles
Yasufumi Kojima • The Astrophysical Journal
(2024)
Magnetar outbursts are powered by an intense magnetic field. The phenomenon has recently drawn significant attention because of a connection to some fast radio bursts that has been reported. Understanding magnetar outbursts may provide the ...
DOAJ
Open Access (DOAJ)
DOI: 10.3847/1538-4357/ad7382
Yunlang Guo, Bo Wang, Xiangdong Li, Dongdong Liu et al. • The Astrophysical Journal
(2025)
Eclipsing millisecond pulsars (MSPs) are a type of pulsar binaries with close orbits (≲1.0 day). They are important objects for studying the accretion history of neutron stars (NSs), pulsar winds, and the origin of isolated MSPs, etc. Recen...
DOAJ
Open Access (DOAJ)
DOI: 10.3847/1538-4357/ae057b
Luciano Rezzolla, P. M. Pizzochero, David Ian Jones, N. Rea et al. • Astrophysics and space science library
(2018)
OPENALEX
DOI: https://doi.org/10.1007/978-3-319-97616-7
FRED HOYLE, William Alfred Fowler, Geoffrey Ronald Burbidge, E. M. Burbidge • The Astrophysical Journal
(1964)
In this paper we have attempted to discuss the relation of massive highly condensed objects to astrolysics in general, rather than only to the radio-source problem. Because situations in which general lativistic effects play a dominant role...
OPENALEX
DOI: https://doi.org/10.1086/147825
Amos Harpaz • A K Peters/CRC Press eBooks
(1993)
A star is by definition a celestial object, bound by self-gravity, in which thermal energy is produced from a nonthermal source (nuclear reactions) and is radiated outward from the object’s surface to its surroundings. We shall extend this ...
OPENALEX
DOI: https://doi.org/10.1201/9781439864678-8
Maria Cristina Baglio, Francesco Coti Zelati, Alessandro Di Marco, Fabio La Monaca et al. • The Astrophysical Journal Letters
(2025)
Transitional millisecond pulsars (tMSPs) bridge the evolutionary gap between accreting neutron stars in low-mass X-ray binaries and millisecond radio pulsars. These systems exhibit a unique subluminous X-ray state characterized by the prese...
DOAJ
Open Access (DOAJ)
DOI: 10.3847/2041-8213/add7d2