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How Massive Single Stars End their Life
A. Heger, C. L. Fryer, S. E. Woosley +2
How massive stars die -- what sort of explosion and remnant each produces -- depends chiefly on the masses of their helium cores and hydrogen envelopes at death. For single stars,…
Massive Star Evolution Through the Ages
A. Heger, S. E. Woosley, C. L. Fryer +1
We review the current basic picture of the evolution of massive stars and how their evolution and structure changes as a function of initial mass. We give an overview of the fate o…
Pristine CNO abundances from Magellanic Cloud B stars I. The LMC cluster NGC 2004 with UVES
A. J. Korn, S. C. Keller, A. Kaufer +4
We present chemical abundances for four main sequence B stars in the young cluster NGC 2004 in the Large Magellanic Cloud (LMC). Apart from H II regions, unevolved OB-type stars ar…