The Origin of Outflows in Evolved Stars (IAU S366)

The prime parameter determining the evolution of a star is its mass, which has large repercussions on its evolutionary path. Low-mass and massive stars power strong stellar winds at the end of their lives, determining the type of stellar end product and contributing to the chemical enrichment of the interstellar medium. IAU Symposium 366 provides an overview of state-of-the-art observational and theoretical studies on the origin of winds in low-mass and massive evolved stars, with topics including binarity, enrichment of the interstellar medium, astrochemistry, and theoretical, observational, and numerical constraints on stellar outflows.

Format: Hardback
Length: 400 pages
Publication date: 19 January 2023
Publisher: Cambridge University Press

The prime factor influencing a star's evolution is its mass, as any alteration to this celestial entity's mass exerts significant consequences on its developmental trajectory. Both low-mass and massive stars are recognized for their ability to generate robust stellar winds during their final stages of existence. These winds play a pivotal role in determining the nature of the stellar end product and the extent to which these stars contribute to the chemical enrichment of the interstellar medium. Ultimately, these winds serve as the fundamental building blocks for the formation of planets and the sustenance of life. A comprehensive grasp of stellar evolution and the fundamental components of the Universe necessitates a thorough comprehension of stellar winds. The International Astronomical Union (IAU) Symposium 366 serves as a comprehensive overview of cutting-edge observational and theoretical investigations into the genesis of winds in low-mass and massive evolved stars. This symposium encompasses a range of topics, including binarity, interstellar medium enrichment, astrochemistry, and theoretical, observational, and numerical constraints on stellar outflows. By delving into these diverse aspects, Symposium 366 aims to shed light on the intricate mechanisms governing the behavior of stars and their impact on the broader cosmos.

Weight: 724g
Dimension: 183 x 253 x 21 (mm)
ISBN-13: 9781108490795