Results 111 to 120 of about 16,242 (188)

Chandra-HETGS Characterization of an Outflowing Wind in the Accreting Millisecond Pulsar IGR J17591–2342 [PDF]

, 2019
Michael A. Nowak, Adamantia Paizis, Gaurava Kumar Jaisawal, Jérôme Chenevez, Sylvain Chaty, Francis Fortin, Jerome Rodriguez, Jörn Wilms, Michael A. Nowak, Adamantia Paizis, Gaurava Kumar Jaisawal, Jérôme Chenevez, Sylvain Chaty, Francis Fortin, Jerome Rodriguez, Jörn Wilms   +15 more
openalex   +1 more source

Intrinsic Emission of PSR B1937+21 at 327 MHz

The Astrophysical Journal
At 327 MHz, the observed emission of PSR B1937+21 is greatly affected by scattering in the interstellar medium, on a timescale of order the pulse period.
Nikhil Mahajan, Marten H. van Kerkwijk
doaj   +1 more source

Millisecond Pulsars, their Evolution and Applications [PDF]

, 2017
R. N. Manchester
openalex   +1 more source

Polarized Multiwavelength Emission from Pulsar Wind—Accretion Disk Interaction in a Transitional Millisecond Pulsar

The Astrophysical Journal Letters
Transitional millisecond pulsars (tMSPs) bridge the evolutionary gap between accreting neutron stars in low-mass X-ray binaries and millisecond radio pulsars.
Maria Cristina Baglio, Francesco Coti Zelati, Alessandro Di Marco, Fabio La Monaca, Alessandro Papitto, Andrew K. Hughes, Sergio Campana, David M. Russell, Diego F. Torres, Francesco Carotenuto, Stefano Covino, Domitilla de Martino, Stefano Giarratana, Sara E. Motta, Kevin Alabarta, Paolo D’Avanzo, Giulia Illiano, Marco M. Messa, Arianna Miraval Zanon, Nanda Rea   +19 more
doaj   +1 more source

Magnetic-distortion-induced Ellipticity and Gravitational Wave Radiation of Neutron Stars: Millisecond Magnetars in Short GRBs, Galactic Pulsars, and Magnetars [PDF]

, 2017
He Gao, Zhoujian Cao, Bing Zhang, He Gao, Zhoujian Cao, Bing Zhang   +5 more
openalex   +1 more source

A Counterintuitive Correlation between Neutron Star Radii Inferred from Pulse Modeling and Surface Emission Beaming

The Astrophysical Journal
Thermal X-ray emission from rotation-powered millisecond pulsars, shaped by gravitational lensing and the beaming of the surface radiation, provides critical insights into neutron star properties. This approach has been the focus of observations with the
Tong Zhao, Dimitrios Psaltis, Feryal Özel   +2 more
doaj   +1 more source

FAST Discovery of Eight Isolated Millisecond Pulsars in NGC 6517

The Astrophysical Journal Letters
We present the discovery of eight isolated millisecond pulsars in globular cluster (GC) NGC 6517 using the Five-hundred-meter Aperture Spherical radio Telescope (FAST).
Dejiang Yin, Li-yun Zhang, Lei Qian, Ralph P. Eatough, Baoda Li, Duncan R. Lorimer, Yinfeng Dai, Yaowei Li, Xingnan Zhang, Minghui Li, Tianhao Su, Yuxiao Wu, Yu Pan, Yujie Lian, Tong Liu, Zhen Yan, Zhichen Pan   +16 more
doaj   +1 more source

Searching for Pulsars in Globular Clusters with the Fast-folding Algorithm and a New Pulsar Discovered in M13

The Astrophysical Journal
We employed the fast-folding algorithm on L -band globular cluster (GC) observations taken with the Five-hundred-meter Aperture Spherical radio Telescope to search for new pulsars, especially those with a long rotational period.
Yaowei Li, Lin Wang, Lei Qian, Liyun Zhang, Yujie Chen, Dejiang Yin, Baoda Li, Yinfeng Dai, Ralph P. Eatough, Wenze Li, Dongyue Jiang, Xingnan Zhang, Minghui Li, Yujie Lian, Yuxiao Wu, Tong Liu, Kuo Liu, Zhichen Pan   +17 more
doaj   +1 more source

Investigating the origin of optical and X-ray pulsations of the transitional millisecond pulsar PSR J1023+0038 [PDF]

, 2022
Giulia Illiano, Alessandro Papitto, Filippo Ambrosino, A. Miraval Zanon, F. Coti Zelati, L. Stella, L. Zampieri, A. Burtovoi, S. Campana, P. Casella, M. Cecconi, D. de Martino, Michele Fiori, A. Ghedina, M. Gonzales, Marcos Hernandez Díaz, G. L. Israel, F. Leone, G. Naletto, Héctor Pérez Ventura, C. Riverol, Luis Riverol, D. F. Torres, Marco Turchetta   +23 more
openalex   +1 more source

Eclipsing Millisecond Pulsars with He Star Companions

The Astrophysical Journal
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.
Yunlang Guo, Bo Wang, Xiangdong Li, Dongdong Liu, Wenshi Tang   +4 more
doaj   +1 more source