Type Ib supernovae are systematically bluer than Type Ic supernovae in optical colors, likely due to helium-rich versus helium-poor progenitors.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
verdicts
UNVERDICTED 2representative citing papers
Frequency analysis of KELT photometry identifies 113 Beta Cephei stars (86 new) plus 96 candidates among known O/B-type stars.
citing papers explorer
-
Type Ib Supernovae are bluer than Type Ic Supernovae
Type Ib supernovae are systematically bluer than Type Ic supernovae in optical colors, likely due to helium-rich versus helium-poor progenitors.
-
New Beta Cephei stars with KELT
Frequency analysis of KELT photometry identifies 113 Beta Cephei stars (86 new) plus 96 candidates among known O/B-type stars.