The carbon star mystery: 40 years later Theory and observations

被引：8

作者：

Straniero, Oscar ^{[1
]}

Abia, Carlos ^{[2
]}

Dominguez, Inma ^{[2
]}

机构：

[1] INAF Osservatorio Astron Abruzzo, Via Maggini Snc, I-64100 Teramo, Italy

[2] Univ Granada, Dept Fis Teor & Cosmos, Granada 18071, Spain

来源：

EUROPEAN PHYSICAL JOURNAL A | 2023年 / 59卷 / 02期

关键词：

GIANT BRANCH STARS; S-PROCESS NUCLEOSYNTHESIS; INTERMEDIATE-MASS STARS; SMALL-MAGELLANIC-CLOUD; CORE HELIUM FLASH; POST-AGB STARS; RED-GIANT; R STARS; CHEMICAL-COMPOSITION; STELLAR MODELS;

D O I：

10.1140/epja/s10050-023-00926-8

中图分类号：

O57 [原子核物理学、高能物理学];

学科分类号：

070202 ;

摘要：

In 1981 Icko Iben Jr published a paper entitled "The carbon star mystery: why do the low mass ones become such, and where have all the high mass ones gone?", where he discussed the discrepancy between the theoretical expectation and its observational counterpart about the luminosity function of AGB carbon stars. After more than 40 years, our understanding of this longstanding problem is greatly improved, also thanks to more refined stellar models and a growing amount of observational constraints. In this paper we review the state of the art of these studies and we briefly illustrate the future perspectives.

引用

页数：10

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