A Red Giants’ Toy Story. II. Understanding the Red-giant Branch Bump

Bibliographic Details
Title: A Red Giants’ Toy Story. II. Understanding the Red-giant Branch Bump
Authors: Marcelo M. Miller Bertolami
Source: The Astrophysical Journal, Vol 943, Iss 1, p 45 (2023)
Publisher Information: IOP Publishing, 2023.
Publication Year: 2023
Collection: LCC:Astrophysics
Subject Terms: Stellar structures, Red giant stars, Stellar interiors, Red giant branch, Red giant bump, Astrophysics, QB460-466
More Details: The Red-Giant Branch Bump (RGBB) is one of the most noteworthy features in the red-giant luminosity function of stellar clusters. It is caused by the passage of the hydrogen-burning shell through the composition discontinuity left at the point of the deepest penetration by the convective envelope. When crossing the discontinuity the usual trend in increasing luminosity reverses for a short time before it increases again, causing a zig-zag in the evolutionary track. In spite of its apparent simplicity the actual physical reason behind the decrease in luminosity is not well understood and several different explanations have been offered. Here we use a recently proposed simple toy model for the structure of low-mass RGs, together with previous results, to show beyond reasonable doubt that the change in luminosity at the RGBB can be traced to the change in the mean molecular weight of the layers on top of the burning shell. And that these changes happen on a nuclear timescale. The change in the effective mean molecular weight, as the burning shell approaches the discontinuity, causes a drop in the temperature of the burning shell which is attenuated by the consequent feedback contraction of the layers immediately below the burning shell. Our work shows that, when applied correctly, including the feedback on the structure of the core together with the increase in the mass of the core, shell-source homology relations do a great quantitative job in explaining the properties of full evolutionary models at the RGBB.
Document Type: article
File Description: electronic resource
Language: English
ISSN: 1538-4357
Relation: https://doaj.org/toc/1538-4357
DOI: 10.3847/1538-4357/acac8a
Access URL: https://doaj.org/article/dd8c9877be3f463790bf499c6026614b
Accession Number: edsdoj.8c9877be3f463790bf499c6026614b
Database: Directory of Open Access Journals
More Details
ISSN:15384357
DOI:10.3847/1538-4357/acac8a
Published in:The Astrophysical Journal
Language:English