Results 121 to 130 of about 43,788 (263)

Timing properties of the X-ray accreting pulsar RX J0440.9+4431 studied with Insight-HXMT and NICER [PDF]

, 2023
P. P. Li, Lian Tao, Y. L. Tuo, Mingyu Ge, Ling-Da Kong, L. Zhang, Qingcui Bu, Long Ji, Jin‐Lu Qu, Shuang‐Nan Zhang, Shuang‐Nan Zhang, Y. Huang, Xiang Ma, W. T. Ye, Qingchang Zhao, Ruican Ma, Shihao Zhao, X. T. Hou, Zi-Xu Yang, Peng-Ju Wang, S. M. Jia, Qing-Cang Shui, Ju Guan   +22 more
openalex   +1 more source

Relativistic Doppler-boosted emission in gamma-ray binaries

, 2010
Gamma-ray binaries could be compact pulsar wind nebulae formed when a young pulsar orbits a massive star. The pulsar wind is contained by the stellar wind of the O or Be companion, creating a relativistic comet-like structure accompanying the pulsar ...
Abdo, Acciari, Acciari, Aharonian, Aharonian, Aharonian, Albert, Albert, Anderhub, Aragona, Arons, B. Cerutti, Bignami, Bogovalov, Bosch-Ramon, Bosch-Ramon, Chernyakova, Chernyakova, Dermer, Dermer, Dubus, Dubus, Dubus, G. Dubus, G. Henri, Georganopoulos, Hinton, Hoffmann, Huang, Kaufman Bernadó, Kennel, Kishishita, Manchester, Maraschi, Martocchia, Motch, Pelling, Reig, Ribó, Takahashi, Tavani   +40 more
core   +3 more sources

Observations of Anomalous X-ray Pulsars [PDF]

, 2001
G. L. Israel, S. Mereghetti, L. Stella
openalex   +1 more source

Magnetic Field Geometry of the Gamma-Ray Binary PSR B1259–63 Revealed via X-Ray Polarization

The Astrophysical Journal Letters
Some X-ray binaries containing an energetic pulsar in orbit around a normal star accelerate particles to high energies in the shock cone formed where the pulsar and stellar winds collide.
Philip Kaaret, Oliver J. Roberts, Steven R. Ehlert, Douglas A. Swartz, Martin C. Weisskopf, Ioannis Liodakis, M. Lynne Saade, Stephen L. O’Dell, Chien-Ting Chen   +8 more
doaj   +1 more source

Two populations of X-ray pulsars produced by two types of supernova [PDF]

, 2011
C. Knigge, M. J. Coe, Philipp Podsiadlowski   +2 more
openalex   +1 more source

X-RAY MEASUREMENT OF THE SPIN-DOWN OF CALVERA: A RADIO- AND GAMMA-RAY-QUIET PULSAR [PDF]

, 2013
J. P. Halpern, S. Bogdanov, E. V. Gotthelf   +2 more
openalex   +1 more source

An X-Ray Synchrotron Shell and a Pulsar: The Peculiar Supernova Remnant G32.4+0.1

The Astrophysical Journal
We present a deep Chandra observation of the shell supernova remnant (SNR) G32.4+0.1, whose featureless X-ray spectrum has led to its classification as an X-ray synchrotron-dominated SNR. We find a partial shell morphology whose outline is quite circular,
Stephen P. Reynolds, Kazimierz J. Borkowski   +1 more
doaj   +1 more source

Non-Thermal X-ray Properties of Rotation Powered Pulsars and Their Wind Nebulae

, 2008
We present a statistical study of the non-thermal X-ray emission of 27 young rotation powered pulsars (RPPs) and 24 pulsar wind nebulae (PWNe) by using the Chandra and the XMM-Newton observations, which with the high spatial resolutions enable us to ...
Becker W., Fang‐Jun Lu, Gil J., Green D. A., Lu T., Lu Y., Roberts D. A., Wei D. M., Xiang‐Hua Li, Zavlin V. E., Zhao Y. H., Zhuo Li   +11 more
core   +2 more sources

X‐Ray Emission from the Planet Pulsar B1257+12 [PDF]

, 2007
G. G. Pavlov, O. Kargaltsev, G. P. Garmire, A. Wolszczan   +3 more
openalex   +1 more source

10 Years of RXTE Monitoring of Five Anomalous X-Ray Pulsars [PDF]

, 2008
Rim Dib, V. M. Kaspi, F. P. Gavriil, C. Bassa, Z. Wang, A. Cumming, V. M. Kaspi   +6 more
openalex   +1 more source