Wave-driven mass loss in the last year of stellar evolution: setting the stage for the most luminous core-collapse supernovae
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnrasl/article-pdf/423/1/L92/9454581/423-1-L92.pdf
Reference26 articles.
1. TOWARD REALISTIC PROGENITORS OF CORE-COLLAPSE SUPERNOVAE
2. Lower mass loss rates in O-type stars: Spectral signatures of dense clumps in the wind of two Galactic O4 stars
3. Pan-STARRS1 DISCOVERY OF TWO ULTRALUMINOUS SUPERNOVAE ATz≈ 0.9
4. A more realistic representation of overshoot at the base of the solar convective envelope as seen by helioseismology
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