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How much H and He is ‘hidden’ in SNe Ib/c? – I. Low-mass objects

MPS-Authors
http://pubman.mpdl.mpg.de/cone/persons/resource/persons22344

Hachinger,  S.
Stellar Astrophysics, MPI for Astrophysics, Max Planck Society;

http://pubman.mpdl.mpg.de/cone/persons/resource/persons4722

Mazzali,  P. A.
Stellar Astrophysics, MPI for Astrophysics, Max Planck Society;

http://pubman.mpdl.mpg.de/cone/persons/resource/persons16154

Taubenberger,  S.
Stellar Astrophysics, MPI for Astrophysics, Max Planck Society;

http://pubman.mpdl.mpg.de/cone/persons/resource/persons4742

Hillebrandt,  W.
Stellar Astrophysics, MPI for Astrophysics, Max Planck Society;

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Citation

Hachinger, S., Mazzali, P. A., Taubenberger, S., Hillebrandt, W., Nomoto, K., & Sauer, D. N. (2012). How much H and He is ‘hidden’ in SNe Ib/c? – I. Low-mass objects. Monthly Notices of the Royal Astronomical Society, 422(1), 70-88. doi:10.1111/j.1365-2966.2012.20464.x.


Cite as: http://hdl.handle.net/11858/00-001M-0000-000F-C363-3
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