Statistical Investigation of Core-Collapse Supernovae and their Host Galaxies

Details Statistical Investigation of Core-Collapse Supernovae and their Host Galaxies Statistical Investigation of Core-Collapse Supernovae and their Host Galaxies

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007jena.confq..53h&link_type=abstract

"JENAM-2007, "Our non-stable Universe", held 20-25 August 2007 in Yerevan, Armenia. Abstract book, p. 53-53"

Statistics

Scientific paper

According to the Padova-Asiago supernova catalogue (up to Sept. 2006) in 243 spiral galaxies with radial velocities smaller than 10000 km/s and with inclination i < 50°, 271 Core-Collapse Supernovae (CCSNe) has been selected. Using methods of two and multi-dimensional statistics the relations between CCSNe (SNe type, galactocentric distance, correlation with spiral arms and HII regions) and their host galaxies (morphology, luminosity, stellar population, neutral hydrogen content etc.) parameters were studied. Main aim of this study is to understand the nature of CCSNe progenitors.

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