Results 91 to 100 of about 706 (178)

Retraction Note to: X-ray observations of PSR B0355+54 and its pulsar wind nebula [PDF]

, 2019
K. McGowan, W. T. Vestrand, J. A. Kennea, Silvia Zane, M. Cropper, F. Cordova   +5 more
openalex   +1 more source

Chandra X-ray Observations of PSR J1849-0001, its Pulsar Wind Nebula, and the TeV Source HESS J1849-000 [PDF]

, 2023
Seth Gagnon, Oleg Kargaltsev, N. J. Klingler, Jeremy Hare, Hui Yang, Alexander Lange, Jordan Eagle   +6 more
openalex   +1 more source

Diagnosing the Particle Transport Mechanism in the Pulsar Halo via X-Ray Observations

The Astrophysical Journal
Pulsar halos (also termed “TeV halos”) are a new class of γ -ray sources in the Galaxy, which manifest as extended γ -ray emission around middle-aged pulsars, as discovered around the Geminga pulsar, the Monogem pulsar, and PSR J0622+3749 by the High ...
Qi-Zuo Wu, Chao-Ming Li, Xuan-Han Liang, Chong Ge, Ruo-Yu Liu   +4 more
doaj   +1 more source

Determination of the energy and kick velocity of Crab Nebula pulsar from the distribution morphology of the remnant

Iraqi Journal of Physics, 2019
Lana T. Ali
doaj   +1 more source

X-Ray Studies of PSR J1838–0655 and its Wind Nebula Associated with HESS J1837–069 and 1LHAASO J1837–0654u

The Astrophysical Journal
We analyzed X-ray data from Chandra, XMM-Newton, NICER, and NuSTAR to characterize the properties of the pulsar PSR J1838−0655 and its pulsar wind nebula (PWN) associated with HESS J1837−069.
Minseo Park, Jaegeun Park, Chanho Kim, Hongjun An   +3 more
doaj   +1 more source

The braking index of PSR B0540−69 and the associated pulsar wind nebula emission after spin-down rate transition [PDF]

, 2020
Ling‐Jun Wang, Mingyu Ge, J. S. Wang, Shanshan Weng, Hao Tong, L. L. Yan, Shuang‐Nan Zhang, Zi-Gao Dai, L. M. Song   +8 more
openalex   +1 more source

Chandra X-Ray Observations of PSR J1849-0001, Its Pulsar Wind Nebula, and the TeV Source HESS J1849-000

The Astrophysical Journal
We obtained a 108 ks Chandra X-ray Observatory (CXO) observation of PSR J1849-0001 and its pulsar wind nebula (PWN) coincident with the TeV source HESS J1849-000.
Seth Gagnon, Oleg Kargaltsev, Noel Klingler, Jeremy Hare, Hui Yang, Alexander Lange, Jordan Eagle   +6 more
doaj   +1 more source

CHANDRAVIEW OF PULSAR WIND NEBULA TORI [PDF]

, 2010
Aya Bamba, Koji Mori, Shinpei Shibata
openalex   +1 more source

High-resolution Radio Study of Pulsar Wind Nebula MSH 15–52 and Supernova Remnant RCW 89

The Astrophysical Journal
We present high-resolution radio observations of the pulsar wind nebula (PWN) MSH 15–5 2 , which is renowned for its distinctive handlike shape, and its associated supernova remnant RCW 89. Using the Australia Telescope Compact Array, we obtained 3 and 6
S. Zhang, C.-Y. Ng, N. Bucciantini
doaj   +1 more source

Subaru Telescope -History, active/adaptive optics, instruments, and scientific achievements. [PDF]

Proc Jpn Acad Ser B Phys Biol Sci, 2021
Iye M.
europepmc   +1 more source