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

Hachinger, S.; Mazzali, P. A.; Taubenberger, S.; Hillebrandt, W.; Nomoto, K.; Sauer, D. N.

doi:10.1111/j.1365-2966.2012.20464.x

Item

ITEM ACTIONSEXPORT

Add to Basket

Local TagsRelease HistoryDetailsSummary

Released

Journal Article

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

MPS-Authors

/persons/resource/persons22344

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

/persons/resource/persons4722

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

/persons/resource/persons16154

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

/persons/resource/persons4742

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

External Resource

No external resources are shared

Fulltext (restricted access)

There are currently no full texts shared for your IP range.

Fulltext (public)

There are no public fulltexts stored in PuRe

Supplementary Material (public)

There is no public supplementary material available

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

Abstract

There is no abstract available