Magnetic Fields in O, B, and A Stars
暫譯: O、B 和 A 型恆星中的磁場

Hubrig, Swetlana, Schöller, Markus

  • 出版商: IOP Publishing Ltd
  • 出版日期: 2021-06-28
  • 售價: $6,400
  • 貴賓價: 9.5$6,080
  • 語言: 英文
  • 頁數: 140
  • 裝訂: Hardcover - also called cloth, retail trade, or trade
  • ISBN: 0750323906
  • ISBN-13: 9780750323901
  • 海外代購書籍(需單獨結帳)

相關主題

商品描述

The last few decades have seen significant progress in our understanding of the occurrence of magnetic fields in stars with radiative envelopes, in particular in massive stars and in intermediate mass stars at early evolutionary stages. This book provides a comprehensive review of the most recent achievements in the measurements of stellar magnetic fields in O, B and A stars. These include the archetypes of stellar magnetism, the chemically peculiar Ap and Bp stars, O- and early B-type stars with their magnetospheres, accreting Herbig Ae/Be stars, Wolf-Rayet stars and high-mass X-ray binaries, among others. It provides an overview of the underlying physics for the interpretation of the data and identifies the requirements, both observational and theoretical, for improving our understanding of the origin of the magnetic fields in early-type stars. It aims to educate scientists working on stars, who are not yet experts in magnetic field studies, assuming that the reader is already familiar with basic terms and concepts of stellar astrophysics.


Key Features


  • Provides a comprehensive review of the field for researchers and students
  • Gives an overview of the underlying physics for the interpretation of data
  • Identifies requirements for understanding the origin of magnetic fields in early-type stars
  • First research-level book on the topic
  • Written by experts in the field of stellar magnetism


商品描述(中文翻譯)

過去幾十年來,我們對於具有輻射包層的恆星中磁場的出現有了顯著的進展,特別是在大質量恆星和早期演化階段的中等質量恆星中。本書提供了對O、B和A型恆星中恆星磁場測量最新成就的全面回顧。這些成就包括恆星磁性原型、化學特異的Ap和Bp恆星、擁有磁層的O型和早期B型恆星、吸積的Herbig Ae/Be恆星、Wolf-Rayet恆星以及高質量X射線雙星等。本書概述了數據解釋的基本物理學,並確定了改善我們對早型恆星磁場起源理解所需的觀測和理論要求。它旨在教育那些尚未成為磁場研究專家的恆星科學家,假設讀者已經熟悉恆星天體物理學的基本術語和概念。

主要特點

- 為研究人員和學生提供該領域的全面回顧
- 概述數據解釋的基本物理學
- 確定理解早型恆星磁場起源的要求
- 該主題的首本研究級別書籍
- 由恆星磁性領域的專家撰寫