Thorne-Żytkow Objects

Fuente: arXiv
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Main Authors: O'Grady, Anna J. G., Moriya, Takashi J., Renzo, Mathieu, Vigna-Gómez, Alejandro
Format: Preprint
Published: 2024
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author O'Grady, Anna J. G.
Moriya, Takashi J.
Renzo, Mathieu
Vigna-Gómez, Alejandro
author_facet O'Grady, Anna J. G.
Moriya, Takashi J.
Renzo, Mathieu
Vigna-Gómez, Alejandro
contents Interacting binary star systems play a critical role in many areas of astrophysics. One interesting example of a binary merger product are Thorne-Żytkow Objects (TŻOs), stars that look like red supergiants but contain neutron stars at their cores. TŻOs were theorized nearly five decades ago, and significant work has gone into understanding the physics of their formation, evolution, and stability. Several searches for TŻO candidates have also been carried out. Whether or not TŻOs could even exist or if they would be stable after formation has also been investigated. Understanding the existence and possible prevalence of TŻOs would have important effects on our understanding of binary evolution, stellar mergers, and inform binary population synthesis models. In this chapter, we review the formation channels, evolution and structure, final fates, and observable signatures of TŻOs, as well as candidates in the literature, from the inception of TŻO theory to recent progress in the field.
format Preprint
id arxiv_https___arxiv_org_abs_2410_02896
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Thorne-Żytkow Objects
O'Grady, Anna J. G.
Moriya, Takashi J.
Renzo, Mathieu
Vigna-Gómez, Alejandro
Solar and Stellar Astrophysics
High Energy Astrophysical Phenomena
Interacting binary star systems play a critical role in many areas of astrophysics. One interesting example of a binary merger product are Thorne-Żytkow Objects (TŻOs), stars that look like red supergiants but contain neutron stars at their cores. TŻOs were theorized nearly five decades ago, and significant work has gone into understanding the physics of their formation, evolution, and stability. Several searches for TŻO candidates have also been carried out. Whether or not TŻOs could even exist or if they would be stable after formation has also been investigated. Understanding the existence and possible prevalence of TŻOs would have important effects on our understanding of binary evolution, stellar mergers, and inform binary population synthesis models. In this chapter, we review the formation channels, evolution and structure, final fates, and observable signatures of TŻOs, as well as candidates in the literature, from the inception of TŻO theory to recent progress in the field.
title Thorne-Żytkow Objects
topic Solar and Stellar Astrophysics
High Energy Astrophysical Phenomena
url https://arxiv.org/abs/2410.02896