SIMBAD references

2018ApJ...864L..35S - Astrophys. J., 864, L35-L35 (2018/September-2)

Red versus blue: early observations of thermonuclear supernovae reveal two distinct populations?

STRITZINGER M.D., SHAPPEE B.J., PIRO A.L., ASHALL C., BARON E., HOEFLICH P., HOLMBO S., HOLOIEN T.W.-S., PHILLIPS M.M., BURNS C.R., CONTRERAS C., MORRELL N. and TUCKER M.A.

Abstract (from CDS):

We examine the early phase intrinsic (B - V)0 color evolution of a dozen SNe Ia discovered within three days of the inferred time of first light (tfirst) and have (B - V)0 color information beginning within five days of tfirst. The sample indicates there are two distinct early populations. The first is a population exhibiting blue colors that slowly evolve, and the second population exhibits red colors and evolves more rapidly. We find that the early blue events are all 1991T/1999aa-like with more luminous, slower declining light curves than those exhibiting early red colors. Placing the first sample on the Branch diagram (i.e., ratio of Si II λλ5972, 6355 pseudo-Equivalent widths) indicates that all blue objects are of the Branch shallow silicon (SS) spectral type, while all early red events except for the 2000cx-like SN 2012fr are of the Branch Core Normal (CN) or CooL (CL) type. A number of potential processes contributing to the early emission are explored, and we find that, in general, the viewing-angle dependance inherent in the companion collision model is inconsistent with all of the SS objects with early-time observations being blue and exhibiting an excess. We caution that great care must be taken when interpreting early phase light curves as there may be a variety of physical processes that are possibly at play and significant theoretical work remains to be done.

Abstract Copyright: © 2018. The American Astronomical Society. All rights reserved.

Journal keyword(s): supernovae: general

CDS comments: Table 1: MUSSES1604D is SN 2016jhr in SIMBAD.

Simbad objects: 26

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