Radio Stars: From kHz to THz
Radio Stars: From kHz to THz
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DOI：
10.1088/1538-3873/aae856
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发表时间：
2018-07
影响因子：
3.5
通讯作者：
L. Matthews
中科院分区：
文献类型：
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作者：
L. Matthews
技术和仪器的进步现在几乎开放了整个无线电频谱来研究恒星。 2017 年 11 月 1 日至 3 日，在麻省理工学院 Haystack 天文台举办了一场名为“射电恒星：从 kHz 到 THz”的国际研讨会，讨论射电波长观测在太阳和恒星天体物理学方面取得的进展。涵盖的主题包括作为无线电明星的太阳；热恒星和冷恒星的射电发射（从主序前到后）；超冷矮星；恒星活动；恒星风和质量损失；行星状星云；灾难性变量；经典新星；以及无线电明星在了解银河系方面的作用。本文总结了会议要点以及一些背景信息。
Advances in technology and instrumentation have now opened up virtually the entire radio spectrum to the study of stars. An international workshop, “Radio Stars: From kHz to THz”, was held at the Massachusetts Institute of Technology Haystack Observatory on 2017 November 1–3 to discuss the progress in solar and stellar astrophysics enabled by radio wavelength observations. Topics covered included the Sun as a radio star; radio emission from hot and cool stars (from the pre- to post-main-sequence); ultracool dwarfs; stellar activity; stellar winds and mass loss; planetary nebulae; cataclysmic variables; classical novae; and the role of radio stars in understanding the Milky Way. This article summarizes meeting highlights along with some contextual background information.