Spatially resolved properties of supernova host galaxies in SDSS-Ⅳ MaNGA

• 作者: Hong-Xuan Zhang Yan-Mei Chen Yong Shi Min Bao Xiao-Ling Yu
• 来源期刊: 天文和天体物理学研究
• 年，卷（期）: 2021,（12）
• 页码范围: 87-99
• 页数: 13页
• 语种: 英文
• DOI: 10.1088/1674-4527/21/12/306

摘要

We crossmatch galaxies from Mapping Nearby Galaxies at Apache Point Observatory with the Open Supernova Catalog,obtaining a total of 132 SNe within MaNGA bundle.These 132 SNe can be classified into 67 Type Ⅰa and 65 Type CC.We study the global and local properties of supernova host galaxies statistically.Type Ⅰa SNe are distributed in both star-forming galaxies and quiescent galaxies,while Type CC SNe are all distributed along the star-forming main sequence.As the stellar mass increases,the Type Ⅰa/CC number ratio increases.We find:(1)there is no obvious difference in the interaction possibilities and environments between Type Ⅰa SN hosts and a control sample of galaxies with similar stellar mass and SFR distributions,except that Type la SNe tend to appear in galaxies which are more bulge-dominated than their controls.For Type CC SNe,there is no difference between their hosts and the control galaxies in galaxy morphology,interaction possibilities as well as environments;(2)compared to galaxy centers,the SN locations have smaller velocity dispersion,lower metallicity,and younger stellar population.This is a natural result of radius gradients for all these parameters.The SN location and its symmetrical position relative to the galaxy center,as well as regions with similar effective radii have very similar[Mg/Fe],gas-phase metallicity,gas velocity dispersion and stellar population age.