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Titlebook: Extrasolar Planets and Their Host Stars; Kaspar von Braun,Tabetha Boyajian Book 2017 Springer International Publishing AG 2017 Exoplanet A

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发表于 2025-3-21 20:00:44 | 显示全部楼层 |阅读模式
书目名称Extrasolar Planets and Their Host Stars
编辑Kaspar von Braun,Tabetha Boyajian
视频video
概述Explains current methods of directly determining astrophysical parameters of exoplanet host stars based on interferometric techniques and how this data provides insights into the exoplanet properties.
丛书名称SpringerBriefs in Astronomy
图书封面Titlebook: Extrasolar Planets and Their Host Stars;  Kaspar von Braun,Tabetha Boyajian Book 2017 Springer International Publishing AG 2017 Exoplanet A
描述This book explores the relations between physical parameters of extrasolar planets and their respective parent stars. Planetary parameters are often directly dependent upon their stellar counterparts. In addition, the star is almost always the only visible component of the system and contains most of the system mass. Consequently, the parent star heavily influences every aspect of planetary physics and astrophysics. Drs. Kaspar von Braun and Tabetha Boyajian use direct methods to characterize exoplanet host starts that minimize the number of assumptions needed to be made in the process..The book provides a background on interferometric techniques for stellar diameter measurements, illustrates the authors‘ approach on using additional data to fully characterize the stars, provides a comprehensive update on the current state of the field, and examines in detail a number of historically significant and well-studied exoplanetary systems..
出版日期Book 2017
关键词Exoplanet Atmospheres; Exoplanets Detectability; Extrasolar Planet Detection; Fundamental Stellar Astro
版次1
doihttps://doi.org/10.1007/978-3-319-61198-3
isbn_softcover978-3-319-61196-9
isbn_ebook978-3-319-61198-3Series ISSN 2191-9100 Series E-ISSN 2191-9119
issn_series 2191-9100
copyrightSpringer International Publishing AG 2017
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发表于 2025-3-21 22:56:57 | 显示全部楼层
Billboards, Planning and Urban Modernism,des to its infrastructure in the next few years and thus open up parameter space currently unavailable to other interferometers. Furthermore, upgrades to CHARA, in particular the installation of an adaptive optics system, in the near future will push CHARA’s limits in both sensitivity and resolution to higher levels.
发表于 2025-3-22 00:51:27 | 显示全部楼层
Book 2017irectly dependent upon their stellar counterparts. In addition, the star is almost always the only visible component of the system and contains most of the system mass. Consequently, the parent star heavily influences every aspect of planetary physics and astrophysics. Drs. Kaspar von Braun and Tabe
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The Determination of Stellar and Planetary Astrophysical Parameters,efly describe our methods used for the direct determination of stellar astrophysical parameters, elaborate on their usefulness, and discuss the applicability of the parameters to other insights into exoplanet science.
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Introduction,ither confirmed or validated, and orders of magnitude more candidates. In fact, there is increasing evidence that there are many more planets in the Milky Way than stars (i.e., > hundreds of billions), particularly in orbit around the significantly more abundant, and arguably much more interesting, low-mass stars.
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