Molecular gas in supernova local environments unveiled by EDGE
CO observations allow estimation of the gas content of molecular clouds, which trace the reservoir of cold gas fuelling star formation, as well as determination of extinction via H2 column density, N(H2). Here, we study millimetric and optical properties at 26 supernovae (SNe) locations of different types in a sample of 23 nearby galaxies, by
Galbany, L. et al.
Fecha de publicación:
3
2017