Model Light Curves for Type Ib and Ic Supernovae

Woosley, S. E.; Sukhbold, Tuguldur; Kasen, D. N.

doi:10.3847/1538-4357/abf3be

Model Light Curves for Type Ib and Ic Supernovae

Journal Article · Fri Jun 04 00:00:00 EDT 2021 · The Astrophysical Journal

DOI:https://doi.org/10.3847/1538-4357/abf3be· OSTI ID:1836260

^[1]; ^[2]; Kasen, D. N. ^[3]

Univ. of California, Santa Cruz, CA (United States)
The Ohio State Univ., Columbus, OH (United States)
Univ. of California, Berkeley, CA (United States); Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)

Using the Monte Carlo code SEDONA, multiband photometry and spectra are calculated for supernovae derived from stripped helium stars with presupernova masses of 2.2 to 10.0 M_⊙. The models are representative of evolution in close binaries and have previously been exploded using a parameterized one-dimensional model for neutrino transport. A subset, those with presupernova masses in the range of 2.2–5.6 M⊙, have many properties in common with observed Type Ib and Ic supernovae, including a median ejected mass near 2 M_⊙, explosion energies near 1 × 10⁵¹ erg, typical ⁵⁶Ni masses of 0.07–0.09 M_⊙, peak times of about 20 days, and a narrow range for the V - R color index 10 days post-V-maximum near 0.3 mag. The median peak bolometric luminosity, near 10^42.3 erg s^-1, is fainter, however, than several observational tabulations, and the brightest explosion has a bolometric luminosity of only 10^42.50 erg s^-1. The brightest absolute B, V, and R magnitudes at peak are -17.2, -17.8, and -18.0. These limits are fainter than some allegedly typical Type Ib and Ic supernovae and could reflect problems in our models or in the observational analysis. Helium stars with lower and higher masses also produce interesting transients that may have been observed, including fast, faint, blue transients and long, red, faint Type Ic supernovae. New models are specifically presented for SN 2007Y, SN 2007gr, SN 2009jf, LSQ 13abf, SN 2008D, and SN 2010X.

View Accepted Manuscript (DOE)

Research Organization:: Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States)

Sponsoring Organization:: USDOE Office of Science (SC), High Energy Physics (HEP)

Grant/Contract Number:: AC02-05CH11231

OSTI ID:: 1836260

Alternate ID(s):: OSTI ID: 23155714

Journal Information:: The Astrophysical Journal, Journal Name: The Astrophysical Journal Journal Issue: 2 Vol. 913; ISSN 0004-637X

Publisher:: IOP PublishingCopyright Statement

Country of Publication:: United States

Language:: English

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