期刊
ASTROPHYSICAL JOURNAL
卷 820, 期 2, 页码 -出版社
IOP PUBLISHING LTD
DOI: 10.3847/0004-637X/820/2/92
关键词
supernovae: general; supernovae: individual (2012cg)
资金
- Hungarian OTKA grant [NN-107637]
- NSF [AST-1109801, AST-1211196, AST-156854]
- NSF Astronomy and Astrophysics Postdoctoral Fellowship [AST-1302771]
- National Science Foundation [NSF PHY-1125915, AST-1008343]
- NSF Graduate Research Fellowship
- NASA Graduate Research Program Fellowship
- NSF STS postdoctoral fellowship [SES-1056580]
- NASA through Space Telescope Science Institute [GO-12540]
- NASA [NAS5-26555, NNX10A196H, UTA13-000844]
- NASA's Astrophysics Data Analysis Program [NNX13AF35G]
- Danish Agency for Science, Technology and Innovation through a Sapere Aude Level 2 grant
- NSF CAREER award [AST-0847157]
- NSF REU grant [PHY-1263280]
- JSPS KAKENHI [26800100]
- MEXT WPI Initiative, Japan
- Direct For Mathematical & Physical Scien
- Division Of Astronomical Sciences [1516854, 1211196, 1302771] Funding Source: National Science Foundation
- Direct For Mathematical & Physical Scien
- Division Of Physics [1263280] Funding Source: National Science Foundation
- Grants-in-Aid for Scientific Research [26800100] Funding Source: KAKEN
We report evidence for excess blue light from the Type Ia supernova (Sn Ia) SN. 2012cg at 15 and 16 days before maximum B-band brightness. The emission is consistent with predictions for the impact of the supernova on a non-degenerate binary companion. This is the first evidence for emission from a companion to a normal SN. Ia. Sixteen days before maximum light, the B - V color of SN. 2012cg is 0.2 mag bluer than for other normal SN. Ia. At later times, this supernova has a typical SN. Ia light curve, with extinction-corrected MB = -19.62 +/- 0.02 mag and Delta m(15)(B)= 0.86 +/- 0.02. Our data set is extensive, with photometry in seven filters from five independent sources. Early spectra also show the effects of blue light, and high-velocity features are observed at early times. Near maximum, the spectra are normal with a silicon velocity v(Si) = -10,500 km s(-1). Comparing the early data with models by Kasen favors a main-sequence companion of about six solar masses. It is possible that many other SN Ia have main-sequence companions that have eluded detection because the emission from the impact is fleeting and faint.
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