XMM-NewtonandSUZAKUdetection of an X-ray emitting shell around the pulsar wind nebula G54.1+0.3

Author:

Bocchino F.,Bandiera R.,Gelfand J.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 25 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. A Pulsar Wind Nebula Origin of the Ultra-high-energy Source 1LHAASO J1929+1846;Research in Astronomy and Astrophysics;2023-09-19

2. Detailed Analysis of the TeV γ-Ray Sources 3HWC J1928+178, 3HWC J1930+188, and the New Source HAWC J1932+192;The Astrophysical Journal;2023-01-01

3. A Spectroscopic Study of Supernova Remnants with the Infrared Space Observatory*;The Astrophysical Journal Supplement Series;2021-11-16

4. Dust masses and grain size distributions of a sample of Galactic pulsar wind nebulae;Monthly Notices of the Royal Astronomical Society;2019-12-06

5. Non-thermal emission and spectral evolution properties of G54.1+0.3;Monthly Notices of the Royal Astronomical Society;2019-06-24

同舟云学术

1.学者识别学者识别

2.学术分析学术分析

3.人才评估人才评估

"同舟云学术"是以全球学者为主线,采集、加工和组织学术论文而形成的新型学术文献查询和分析系统,可以对全球学者进行文献检索和人才价值评估。用户可以通过关注某些学科领域的顶尖人物而持续追踪该领域的学科进展和研究前沿。经过近期的数据扩容,当前同舟云学术共收录了国内外主流学术期刊6万余种,收集的期刊论文及会议论文总量共计约1.5亿篇,并以每天添加12000余篇中外论文的速度递增。我们也可以为用户提供个性化、定制化的学者数据。欢迎来电咨询!咨询电话:010-8811{复制后删除}0370

www.globalauthorid.com

TOP

Copyright © 2019-2024 北京同舟云网络信息技术有限公司
京公网安备11010802033243号  京ICP备18003416号-3