Results 111 to 120 of about 31,557 (257)

The Radio-bright Accreting Millisecond X-Ray Pulsar IGR J17591-2342 [PDF]

, 2018
T. D. Russell, N. Degenaar, R. Wijnands, J. van den Eijnden, N. V. Gusinskaia, J. W. T. Hessels, J. C. A. Miller-Jones   +6 more
openalex   +1 more source

On the beam properties of radio pulsars with interpulse emission [PDF]

, 2019
S. Johnston, M. Krämer
openalex   +1 more source

Energetic Young Radio Pulsars [PDF]

, 1998
12 pages, Latex, requires aaspp4.sty, 4 postscript figures, Invited review to appear in: The Many Faces of Neutron Stars, Proceedings of the NATO ASI conference, Lipari, Eolian Islands, 1-10 October ...
openaire   +2 more sources

Single-pulse Morphology of PSR J1935+1616 (B1933+16) Based on Archival Data from FAST

The Astrophysical Journal
We utilized archive data from the Five-hundred-meter Aperture Spherical Radio Telescope (FAST) to analyze the single-pulse profile morphology of PSR J1935+1616 (B1933+16).
R. W. Tian, R. S. Zhao, Marilyn Cruces, H. Liu, D. Li, P. Wang, C. H. Niu, Biping Gong, C. C. Miao, X. Zhu, H. W. Xu, W. L. Li, S. D. Wang, Z. F. Tu, Q. J. Zhi, S. J. Dang, L. H. Shang, S. Xiao   +17 more
doaj   +1 more source

Rotational Evolution of the Slowest Radio Pulsar, PSR J0250+5854 [PDF]

, 2019
F. F. Kou, Hao Tong, Renxin Xu, Xia Zhou
openalex   +1 more source

China's 'sky eye': exploring the universe by measuring faint cosmic radio signals. [PDF]

Natl Sci Rev, 2023
Zhao W.
europepmc   +1 more source

Kinematics of Radio Pulsars [PDF]

, 2001
For the proceedings of the NATO-ASI, held in Crete, Greece, from 7-18 June ...
openaire   +2 more sources

A binary pulsar in a 53-minute orbit. [PDF]

Nature, 2023
Pan Z, Lu JG, Jiang P, Han JL, Chen HL, Han ZW, Liu K, Qian L, Xu RX, Zhang B, Luo JT, Yan Z, Yang ZL, Zhou DJ, Wang PF, Wang C, Li MH, Zhu M.   +17 more
europepmc   +1 more source

Polarimetry of 600 pulsars from observations at 1.4 GHz with the Parkes radio telescope [PDF]

, 2017
S. Johnston, M. Kerr
openalex   +1 more source

Timing of Millisecond Pulsars in NGC 6752. III. On the Presence of Nonluminous Matter in the Cluster’s Core

The Astrophysical Journal
Millisecond pulsars are subject to accelerations in globular clusters (GCs) that manifest themselves in both the first and second spin period time derivatives, and can be used to explore the mass distribution of the potentials they inhabit.
A. Corongiu, A. Ridolfi, F. Abbate, M. Bailes, A. Possenti, M. Geyer, R. N. Manchester, M. Kramer, P. C. C. Freire, M. Burgay, S. Buchner, F. Camilo   +11 more
doaj   +1 more source