ISSN:
1476-4687
Source:
Nature Archives 1869 - 2009
Topics:
Biology
,
Chemistry and Pharmacology
,
Medicine
,
Natural Sciences in General
,
Physics
Notes:
[Auszug] To account for the lack (or weakness) of hydrogen and helium features in type Ic supernovae, massive (C + O)-rich stars have been suggested for the progenitors4. The difficulty with such massive-star models may be that the decline of the calculated light curve is significantly slower ...
Type of Medium:
Electronic Resource
URL:
http://dx.doi.org/10.1038/371227a0
Permalink