Progenitor mass constraints for the type Ib intermediate-luminosity SN 2015ap and the highly extinguished SN 2016bau. Issue 2 (14th May 2021)

• Record Type: Journal Article
• Authors: Aryan, Amar; Pandey, S B; Zheng, WeiKang; Filippenko, Alexei V; Vinko, Jozsef; Ouchi, Ryoma; Shivvers, Isaac; Yuk, Heechan; Kumar, Sahana; Stegman, Samantha; Halevi, Goni; Ross, Timothy W; Gould, Carolina; Yunus, Sameen; Baer-Way, Raphael; deGraw, Asia; Maeda, Keiichi; Bhattacharya, D; Kumar, Amit; Gupta, Rahul; Yadav, Abhay P; Buckley, David A H; Misra, Kuntal; Tiwari, S N
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 505:Issue 2(2021)
• Page Start: 2530
• Page End: 2547
• Publication Date: 2021-05-14
• Subjects: techniques: photometric -- techniques: spectroscopic -- supernovae: general -- supernovae: individual: SN 2016bau, SN 2015ap; Astronomy -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnras/stab1379
• Languages: English
• ISSNs: 0035-8711

Abstract

ABSTRACT: Photometric and spectroscopic analyses of the intermediate-luminosity Type Ib supernova (SN) 2015ap and of the heavily reddened Type Ib SN 2016bau are discussed. Photometric properties of the two SNe, such as colour evolution, bolometric luminosity, photospheric radius, temperature, and velocity evolution, are also constrained. The ejecta mass, synthesized nickel mass, and kinetic energy of the ejecta are calculated from their light-curve analysis. We also model and compare the spectra of SN 2015ap and SN 2016bau at various stages of their evolution. The P Cygni profiles of various lines present in the spectra are used to determine the velocity evolution of the ejecta. To account for the observed photometric and spectroscopic properties of the two SNe, we have computed 12 M⊙ zero-age main-sequence (ZAMS) star models and evolved them until the onset of core-collapse using the publicly available stellar-evolution codeMESA . Synthetic explosions were produced using the public version of STELLA and another publicly available code, SNEC, utilizing the MESA models. SNEC and stella provide various observable properties such as the bolometric luminosity and velocity evolution. The parameters produced by SNEC /STELLA and our observations show close agreement with each other, thus supporting a 12 M⊙ ZAMS star as the possible progenitor for SN 2015ap, while the progenitor of SN 2016bau is slightly less massive, being close to the boundary between SN and non-SN as the final product.