Gamma ray heating rates due to chromium isotopes in stellar core during late stages of high mass stars (>10M)

Publisher: Edp Sciences

E-ISSN: 2100-014x|154|issue|01005-01005

ISSN: 2100-014x

Source: EPJ Web of Conference, Vol.154, Iss.issue, 2017-09, pp. : 01005-01005

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Abstract