On the significance of steady mass loss in red giants prior to envelope ejection due to pulsational instability

Details On the significance of steady mass loss in red giants prior to envelope ejection due to pulsational instability On the significance of steady mass loss in red giants prior to envelope ejection due to pulsational instability

Apr 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...237..105b&link_type=abstract

Astrophysical Journal, Part 1, vol. 237, Apr. 1, 1980, p. 105-110.

Statistics

16

Red Giant Stars, Stellar Envelopes, Stellar Mass Ejection, Variable Stars, Planetary Nebulae, Stellar Evolution

Scientific paper

Reimers-type steady mass loss is shown to have a modest effect on Mira
variable evolution. Up to the point where envelope ejection due to
pulsational instability occurs, only a small fraction of the envelope
can be lost as a result of steady mass loss. The effects of steady mass
loss on Mira variable statistics are discussed.

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