Intrinsic color diversity of nearby Type Ia supernovae

被引:3
作者
Arima, Noriaki [1 ,2 ]
Doi, Mamoru [1 ,3 ,4 ]
Morokuma, Tomoki [1 ]
Takanashi, Naohiro [5 ]
机构
[1] Univ Tokyo, Grad Sch Sci, Inst Astron, 2-21-1 Osawa, Mitaka, Tokyo 1810015, Japan
[2] Univ Tokyo, Grad Sch Sci, Dept Astron, Bunkyo Ku, 7-3-1 Hongo, Tokyo 1130033, Japan
[3] Univ Tokyo, Res Ctr Early Universe, Grad Sch Sci, Bunkyo Ku, 7-3-1 Hongo, Tokyo 1130033, Japan
[4] Univ Tokyo, Kavli Inst Phys & Math Universe, 5-1-5 Kashiwanoha, Kashiwa, Chiba 2778583, Japan
[5] Univ Tokyo, Execut Management Program, Bunkyo Ku, 7-3-1 Hongo, Tokyo 1138654, Japan
基金
日本学术振兴会;
关键词
dust; extinction; galaxies: general; supernovae: general; LIGHT-CURVE; HUBBLE RESIDUALS; PROJECT; METALLICITY; MODELS; DUST; CONSTRAINTS; PHOTOMETRY; EVOLUTION; RADIATION;
D O I
10.1093/pasj/psaa123
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
It has been reported that the extinction law for Type Ia supernovae (SNe Ia) may be different from the one in the Milky Way, but the intrinsic color of SNe Ia and the dust extinction are observationally mixed. In this study, we examine photometric properties of SNe Ia in the nearby universe (z less than or similar to 0.04) to investigate the SN Ia intrinsic color and the dust extinction. We focus on the Branch spectroscopic classification of 34 SNe Ia and morphological types of host galaxies. We carefully study the distribution of their peak colors on the B - V, V - R color-color diagram, as well as the color excess and absolute magnitude deviation from the stretch-color relation of the bluest SNe Ia. We find that SNe Ia which show the reddest color occur in early-type spirals and the trend holds when divided into Branch sub-types. The dust extinction becomes close to the Milky Way like extinction if we exclude some peculiar red Broad Line (BL) sub-type SNe Ia. Furthermore, two of these red BLs occur in elliptical galaxies, a less-dusty environment, suggesting intrinsic color diversity in BL sub-type SNe Ia.
引用
收藏
页码:326 / 337
页数:12
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