The C/N ratio and N-14 abundance as tests of the theories of Wolf-Rayet stars formation

Details The C/N ratio and N-14 abundance as tests of the theories of Wolf-Rayet stars formation The C/N ratio and N-14 abundance as tests of the theories of Wolf-Rayet stars formation

Jan 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981a%26a....94l...1g&link_type=abstract

Astronomy and Astrophysics, vol. 94, no. 1, Jan. 1981, p. L1, L2.

Astronomy and Astrophysics

Astrophysics

15

Abundance, Carbon, Nitrogen, Stellar Evolution, Stellar Mass Ejection, Wolf-Rayet Stars, Helium, Ratios

Scientific paper

A widely accepted scheme for WR stars formation is that they result from
mass loss from normal stars. This theory predicts strong constraints on
the C/N ratio. This should permit a good check of its validity. In that
theory, C/N is always of the order of 0.02 in WN and N/C is always
smaller than 0.000001 in WC stars and is zero in most of them.

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