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High-Mass X-Ray Binaries (Iau S346): Illuminating the Passage from Massive Binaries to Merging Compact Objects

High-mass X-ray Binaries (IAU S346)

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"High-mass X-ray Binaries (IAU S346)" by Lidia M. Oskinova, Enrico Bozzo, Tomasz Bulik, Douglas R. Gies is a astronomy book and space science reference focused on Deep Sky & Solar System. Best for students, researchers, and serious astronomy enthusiasts.

Providing an up-to-date overview of research in the field of high-mass X-ray binaries, this volume consists of the contributions made at IAU Symposium 346. Taking an interdisciplinary approach, it includes reviews on massive star winds and HMXB donors, Be Stars in the X-ray binary context, dynamical versus isolated formation channels of gravitational-wave sources, HMXBs as progenitors of double compact objects, HMXBs in the Early Universe and their impact in cosmology and gravitational wave astrophysics, as well as the summary review 'High Mass X-ray Binaries: Beacons in a Stormy Universe'. This Symposium provides a bridge between the relatively mature field of massive binary astrophysics and the newly emerging field of gravitational wave astronomy, indicating the future development of this growing branch of astrophysics. It is essential reading for graduate students and researchers who are looking to gain a general overview of current research activity on X-ray binaries.

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Best For: Researchers and students in astrophysics focusing on high-mass X-ray binaries and related phenomena.
Focus: Current research and interdisciplinary reviews on high-mass X-ray binaries, including massive star winds, Be stars, formation channels of gravitational-wave sources, and early universe HMXBs.
Covers: Massive star winds, HMXB donor stars, Be stars in X-ray binaries, formation of gravitational-wave sources, progenitors of double compact objects, and HMXBs in the early universe.
Why It Matters: It consolidates recent findings and diverse perspectives on high-mass X-ray binaries, aiding understanding of their role in stellar evolution and gravitational-wave source formation.

"High-mass X-ray Binaries (IAU S346)" by Lidia M. Oskinova, Enrico Bozzo, Tomasz Bulik, Douglas R. Gies is a astronomy book and space science reference focused on Deep Sky & Solar System. Best for students, researchers, and serious astronomy enthusiasts.

Topic: Deep Sky & Solar System

Author: Lidia M. Oskinova, Enrico Bozzo, Tomasz Bulik, Douglas R. Gies

Who this is for:

  • Astronomy students
  • Researchers and advanced hobbyists
  • Readers exploring space science topics

Why this book matters: It matters because it helps readers build a stronger understanding of astronomy concepts, observations, and scientific ideas related to space.

Providing an up-to-date overview of research in the field of high-mass X-ray binaries, this volume consists of the contributions made at IAU Symposium 346. Taking an interdisciplinary approach, it includes reviews on massive star winds and HMXB donors, Be Stars in the X-ray binary context, dynamical versus isolated formation channels of gravitational-wave sources, HMXBs as progenitors of double compact objects, HMXBs in the Early Universe and their impact in cosmology and gravitational wave astrophysics, as well as the summary review 'High Mass X-ray Binaries: Beacons in a Stormy Universe'. This Symposium provides a bridge between the relatively mature field of massive binary astrophysics and the newly emerging field of gravitational wave astronomy, indicating the future development of this growing branch of astrophysics. It is essential reading for graduate students and researchers who are looking to gain a general overview of current research activity on X-ray binaries.

AuthorLidia M. Oskinova, Enrico Bozzo, Tomasz Bulik, Douglas R. Gies
PublisherCambridge University Press
Published2020-01-31
ISBN-139781108471589
BindingHardcover
Pages500
LanguageEnglish
SubjectsScience
TopicDeep Sky & Solar System
SeriesProceedings of the International Astronomical Union Symposia

Format: Hardcover

Length: 500 pages

Language: English

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