Star formation in the early universe

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

In low-metallicity environments, massive stars are more easily formed than in the solar neighborhood. In this article, we see the following examples of low-mass star formation. We first describe the first star formation in the universe and argue that they are typically ordinary-sized massive stars, rather than very massive (> 100M ·) ones. Next, we see how the metal-enrichment changes the thermal evolution of gas, thereby causing the shift of characteristic stellar mass towards lower mass. Finally, we discuss the possibility of forming supermassive stars in some special conditions in young galaxies.

Original languageEnglish
Title of host publicationDeath of Massive Stars
Subtitle of host publicationSupernovae and Gamma-Ray Bursts
EditorsPeter W. A. San Antonio, Nobuyuki Kawai, Elena Pian
Pages216-223
Number of pages8
EditionS279
DOIs
Publication statusPublished - 2011 Apr

Publication series

NameProceedings of the International Astronomical Union
NumberS279
Volume7
ISSN (Print)1743-9213
ISSN (Electronic)1743-9221

Keywords

  • Pop II Stars
  • Pop III Stars
  • Star Formation

ASJC Scopus subject areas

  • Medicine (miscellaneous)
  • Astronomy and Astrophysics
  • Nutrition and Dietetics
  • Public Health, Environmental and Occupational Health
  • Space and Planetary Science

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