Results 101 to 110 of about 800,901 (220)

PSR J1914+2636: Quasiperiodic Nulling and Bright-pulse Emission from an Old Pulsar in the Death Valley

The Astrophysical Journal
In this paper, we report high-sensitivity single-pulse observations of PSR J1914+2636 using the Five-hundred-meter Aperture Spherical radio Telescope (FAST).
Yi-feng Peng, Shi-jun Dang, Qing-dong Wu, Wei-Yang Wang, Yu-bing Wang, Zu-rong Zhou, Yin-wen Gong, Qi-jun Zhi, Wei Li   +8 more
doaj   +1 more source

Gamma-ray pulsars with Fermi

, 2016
International audienceIn 8 years of operation, the Large Area Telescope (LAT) on the Fermi satellite has impacted our understanding of gamma-ray pulsars dramatically.
Barr, Ewan, Lucas Guillemot, Ewan Barr, Smith, David A., Matthew Kerr, Guillemot, Lucas, Kerr, Matthew, Ng, Cherry, David Smith, Cherry Ng   +9 more
core   +1 more source

On the decay of the magnetic fields of single radio pulsars [PDF]

, 1992
We investigate the statistical evidence for the decay of the magnetic field of single radio pulsars. We perform population syntheses for different assumed values for the time scale of field decay using a Monte Carlo method.
Wijers, R.A.M.J., Verbunt, F., Hartman, J.W., Bhattacharya, D.   +3 more
core   +2 more sources

Identifying Pulsar Candidates in Interferometric Radio Images Using Scintillation

The Astrophysical Journal
Pulsars have been primarily detected by their narrow pulses or periodicity in time domain data. Interferometric surveys for pulsars are challenging due to the trade-off between beam sensitivity and beam size and the corresponding tradeoff between survey ...
Jitendra Salal, Shriharsh P. Tendulkar, Visweshwar Ram Marthi   +2 more
doaj   +1 more source

Fast Radio Bursts from Monster Shocks and Flares of Inspiraling Binary Neutron Stars: A Kinetic Model for Double Pulsar [PDF]

Jan Benáček, Benoît Cerutti, MARTIN POHL, Tim Dietrich, Anna Neuweiler   +4 more
openalex   +1 more source

Two radio pulsars with magnetar fields

, 2004
PSRs J1847-0130 and J1718-37184 have inferred surface dipole magnetic fields greater than those of any other known pulsars and well above the "quantum critical field" above which some models predict radio emission should not occur. These fields
Lyne AG, Faulkner AJ, Manchester RN, D'AMICO, NICOLO', Camilo F, Kramer M, Stairs IH, McLaughlin MA, Kaspi VM, Hobbs G, Lorimer DR, Possenti A   +11 more
core  

Radio pulsars and transients in the Galactic center

, 2006
Radio pulsars and transients provide powerful probes of the star formation history, interstellar medium, and gravitational potential of the Galactic center.
J. S. Deneva (19104848), D. C. Backer (19127029), W. Vlemmings (19009409), Scott D. Hyman (19127026), P. Demorest (19001309), Joseph Lazio (10290275), Geoffrey C. Bower (5992391), J. M. Cordes (19001237), R. Bhat (4744917), S. Chatterjee (2314663), S. M. Ransom (19005266)   +10 more
core   +1 more source

Follow-up Investigation of 11 Pulsars Discovered in the Commensal Radio Astronomy FAST Survey

The Astrophysical Journal
In this paper, we study 11 pulsars that were discovered by the Five-hundred-meter Aperture Spherical radio Telescope (FAST) in the Commensal Radio Astronomy FAST Survey.
K. Yang, L. Li, J. P. Yuan, N. Wang, D. Li, P. Wang, C. C. Miao, W. W. Zhu, M. Y. Xue, W. M. Yan, J. B. Wang, R. Yuen, G. L. Lü, C. H. Zhu, J. M. Yao, Q. D. Wu, S. Q. Wang, S. N. Sun, F. F. Kou, D. Zhao, Z. Wang, J. Xu, C. Sun, Y. Feng, Z. J. Liu, X. L. Miao, L. Q. Meng, C. H. Niu, J. R. Niu, L. Qian, X. Y. Xie, Y. F. Xiao, Y. L. Yue, S. P. You, S. J. Dang, X. H. Yu, R. S. Zhao, X. Zhou, L. Zhang, J. F. Wu, C. J. Wang, Y. B. Wang, Z. Y. Gan   +42 more
doaj   +1 more source

A survey for radio pulsars and transients in the 10 pc region around Sgr A*

Astronomy & Astrophysics
Here we report on a new survey for pulsars and transients in the 10 pc region around Sgr A∗ using the Effelsberg radio telescope at frequencies between 4 and 8 GHz.
Desvignes G., Eatough R. P., Men Y. P., Abbate F., Karuppusamy R., Kramer M., Liu K., Shao L., Torne P., Wharton R. S.   +9 more
doaj   +1 more source

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