Does Metallicity Affect the Fate of Massive Stars?
TypeCapitulo de libro
Conicyt InstrumentCentros de Investigación en Áreas Prioritarias
We are working to answer this question by measuring abundances of HII regions in galaxies that hosted Core Collapse Supernovae (CCSNe), and correlating them with the SN properties. The latter will be derived for 63 nearby (z < 0.08) CCSNe with high qualit
American Astronomical Society Meeting