ASASSN-18tb: A most unusual Type Ia supernova observed by TESS and SALT

Abstract

We present photometric and spectroscopic observations of the unusual Type Ia supernova ASASSN-18tb, including a series of Southern African Large Telescope spectra obtained over the course of nearly six months and the first observations of a supernova by the Transiting Exoplanet Survey Satellite.We confirm a previous observation by Kollmeier et al. showing that ASASSN-18tb is the first relatively normal Type Ia supernova to exhibit clear broad (~1000 km s-1) Hα emission in its nebular-phase spectra.We find that this event is best explained as a sub- Chandrasekhar mass explosion producing MNi ≈ 0.3 M⊙. Despite the strong Hα signature at late times, we find that the early rise of the supernova shows no evidence for deviations from a single-component power-law and is best fit with a moderately shallow power law of index 1.69 ± 0.04. We find that the Hα luminosity remains approximately constant after its initial detection at phase +37 d, and that the Hα velocity evolution does not trace that of the Fe III λ4660 emission. These suggest that the Hα emission arises from a circumstellar medium (CSM) rather than swept-up material from a non-degenerate companion. However, ASASSN- 18tb is strikingly different from other known CSM-interacting Type Ia supernovae in a number of significant ways. Those objects typically show an Hα luminosity two orders of magnitude higher than what is seen in ASASSN-18tb, pushing them away from the empirical light-curve relations that define 'normal' Type Ia supernovae. Conversely, ASASSN-18tb exhibits a fairly typical light curve and luminosity for an underluminous or transitional SN Ia, with MR ≈ -18.1 mag. Moreover, ASASSN-18tb is the only SN Ia showing Hα from CSM interaction to be discovered in an early-type galaxy.