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Cited by 18Astrophysics and Star Formation StudiesStellar, planetary, and galactic studiesAstro and Planetary Science

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Number of stars in the Sun’s birth cluster revisited

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Arakawa, Sota, Kokubo, Eiichiro·2023·Astronomy & Astrophysics
DOI 10.1051/0004-6361/202244743
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Abstract

The Sun is thought to have been formed within a star cluster. The coexistence of 26 Al-rich and 26 Al-poor calcium–aluminum-rich inclusions indicates that a direct injection of 26 Al-rich materials from a nearby core-collapse supernova would be expected to occur in the first 10 5 years of the existence of the Solar System. Therefore, at least one core-collapse supernova ought to occur within the duration of star formation in the Sun’s birth cluster. Here, we revisit the number of stars in the Sun’s birth cluster from the point of view of the probability of experiencing at least one core-collapse supernova within the finite duration of star formation within the birth cluster. We find that the number of stars in the birth cluster may be significantly greater than that previously considered, depending on the duration of star formation.

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Metadata

Authors
Arakawa, S., & Kokubo, E.
Affiliations
  • Japan Agency for Marine-Earth Science and Technology (JP)
  • National Astronomical Observatory of Japan (JP)
ORCID
Venue
Astronomy & Astrophysics
Publisher
EDP Sciences
Published
2023-02
Volume
670
Pages
A105
ISSN
  • 0004-6361 (ISSN-L)
  • 1432-0746
DOI
10.1051/0004-6361/202244743
OpenAlex
W4315631752
Cited by
18
References
4
Citations by year
2026: 1 · 2025: 7 · 2024: 7 · 2023: 3
FWCI
2.10
Type
journal article
Language
en
Open access
Licence
Locations
  • Astronomy and Astrophysics (publishedVersion, cc-by)
  • arXiv (Cornell University) (submittedVersion)
  • Springer Link (Chiba Institute of Technology) (submittedVersion)
  • arXiv (Cornell University)
Funders
Japan Society for the Promotion of Science (JP20J00598, 18H05438)
Topics
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astrophysics and Star Formation Studies
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
  • Physical Sciences › Earth and Planetary Sciences › Space and Planetary Science › Astro and Planetary Science
Keywords
core-collapse supernovae, calcium-aluminum-rich inclusions, 26Al, cluster size, solar system formation

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