Non-thermal radio emission from O-type stars
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361/200913450/pdf
Reference49 articles.
1. A Steady, Radiative‐Shock Method for Computing X‐Ray Emission from Colliding Stellar Winds in Close, Massive‐Star Binaries
2. The acceleration of cosmic rays in shock fronts - I
3. Turbulent amplification of magnetic field and diffusive shock acceleration of cosmic rays
4. A survey of radio emission from Galactic OB stars
Cited by 27 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. MOBSTER – VI. The crucial influence of rotation on the radio magnetospheres of hot stars;Monthly Notices of the Royal Astronomical Society;2022-04-27
2. AU-scale radio imaging of the wind collision region in the brightest and most luminous non-thermal colliding wind binary Apep;Monthly Notices of the Royal Astronomical Society;2020-12-16
3. COBRaS: The e-MERLIN 21 cm Legacy survey of Cygnus OB2;Astronomy & Astrophysics;2020-05
4. Search for non-thermal X-ray emission in the colliding wind binary Cygnus OB2 #8A;Astronomy & Astrophysics;2020-04
5. Megahertz emission of massive early-type stars in the Cygnus region;Publications of the Astronomical Society of Australia;2020
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