Circumstellar disks in high-mass star environments: the early solar system

Details Circumstellar disks in high-mass star environments: the early solar system Circumstellar disks in high-mass star environments: the early solar system

Nov 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010hia....15..746m&link_type=abstract

Highlights of Astronomy, Volume 15, p. 746-747

Astronomy and Astrophysics

Astronomy

1

Early Solar System, Meteorites, Nucleosynthesis, Massive Stars

Scientific paper

The early solar system represents the only case we have of a circumstellar disk that can be investigated “in situ” -albeit 4.6 Gyr after its formation. Meteorites studies give mounting evidence for an intense irradiation phase of the young circumsolar disk by energetic particles, and also for contamination by products of high-mass stellar and/or explosive nucleosynthesis. We thus discuss the conditions of the birth of the solar system in a high-mass star environment.

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