Bibcode
Galbany, L.; Stanishev, V.; Mourão, A. M.; Rodrigues, M.; Flores, H.; García-Benito, R.; Mast, D.; Mendoza, M. A.; Sánchez, S. F.; Badenes, C.; Barrera-Ballesteros, J.; Bland-Hawthorn, J.; Falcón-Barroso, J.; García-Lorenzo, B.; Gomes, J. M.; González Delgado, R. M.; Kehrig, C.; Lyubenova, M.; López-Sánchez, A. R.; de Lorenzo-Cáceres, A.; Marino, R. A.; Meidt, S.; Mollá, M.; Papaderos, P.; Pérez-Torres, M. A.; Rosales-Ortega, F. F.; van de Ven, G.
Bibliographical reference
Astronomy and Astrophysics, Volume 572, id.A38, 24 pp.
Advertised on:
12
2014
Journal
Citations
108
Refereed citations
99
Description
We use optical integral field spectroscopy (IFS) of nearby supernova
(SN) host galaxies (0.005 2.4 Gyr, respectively) than
the massive SN Ia hosts (0.04%, 2.01%, and 97.95% in these intervals).
We estimate that the low-mass galaxies produce ten times fewer SNe Ia
and three times fewer CC SNe than the high-mass group. Therefore the
ratio between the number of CC SNe and SNe Ia is expected to increase
with decreasing galaxy mass. CC SNe tend to explode at positions with
younger stellar populations than the galaxy average, but the galaxy
properties at SNe Ia locations are one average the same as the global
galaxy properties.
Tables 2, 3, 7-9 are only available in electronic form at http://www.aanda.org
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