PTF11mnb Bgri light curves

DOI

We study PTF11mnb, a He-poor supernova (SN) whose light curves resemble those of SN 2005bf, a peculiar double-peaked stripped-envelope (SE) SN, until the declining phase after the main peak. We investigate the mechanism powering its light curve and the nature of its progenitor star. Optical photometry and spectroscopy of PTF11mnb are presented. We compared light curves, colors and spectral properties to those of SN 2005bf and normal SE SNe. We built a bolometric light curve and modeled this light curve with the SuperNova Explosion Code (SNEC) hydrodynamical code explosion of a MESA progenitor star and semi-analytic models.

Identifier
DOI http://doi.org/10.26093/cds/vizier.36090106
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/609/A106
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/609/A106
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/609/A106
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/609/A106
Provenance
Creator Taddia F.; Sollerman J.; Fremling C.; Karamehmetoglu E.; Quimby R.M.,Gal-Yam A.; Yaron O.; Kasliwal M.M.; Kulkarni S.R.; Nugent P.E.; Smadja G.,Tao C.
Publisher CDS
Publication Year 2018
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy