X-RAY OBSERVATIONS OF THE SUPERNOVA REMNANT CTB 87 (G74.9+1.2): AN EVOLVED PULSAR WIND NEBULA-Reference-Cited by-同舟云学术

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X-RAY OBSERVATIONS OF THE SUPERNOVA REMNANT CTB 87 (G74.9+1.2): AN EVOLVED PULSAR WIND NEBULA

Published:2013-08-13 Issue:1 Volume:774 Page:33
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Matheson H.,Safi-Harb S.,Kothes R.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/774/i=1/a=33/pdf

Reference38 articles.

1. Discovery of TeV Gamma-Ray Emission from the Cygnus Region of the Galaxy

2. First detection of a VHE gamma-ray spectral maximum from a cosmic source: HESS discovery of the Vela X nebula

3. DISCOVERY OF AN ENERGETIC PULSAR ASSOCIATED WITH SNR G76.9+1.0

Cited by 22 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Discovery and timing of pulsar J2016+3711 in supernova remnant CTB 87 with FAST;Monthly Notices of the Royal Astronomical Society;2024-02-05

2. On the plerionic rectangular supernova remnants of static progenitors;Monthly Notices of the Royal Astronomical Society;2023-11-15

3. Radio Emission Spectrum of Supernova Remnant G74.9+1.2;Astronomy Reports;2023-10

4. RADIO EMISSION SPECTRUM OF COMPOSITE SUPERNOVA REMNANT G74.9+1.2;Астрономический журнал;2023-10-01

5. Extended radio halo of the supernova remnant CTB87 (G74.9+1.2);Astronomy & Astrophysics;2022-12

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