A1 Refereed original research article in a scientific journal

Studying the environment of AT2018cow with MUSE




AuthorsLyman JD, Galbany L, Sanchez SF, Anderson JP, Kuncarayakti H, Prieto JL

PublisherOXFORD UNIV PRESS

Publication year2020

JournalMonthly Notices of the Royal Astronomical Society

Journal name in sourceMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY

Journal acronymMON NOT R ASTRON SOC

Volume495

Issue1

First page 992

Last page999

Number of pages8

ISSN0035-8711

eISSN1365-2966

DOIhttps://doi.org/10.1093/mnras/staa1243

Self-archived copy’s web addresshttps://research.utu.fi/converis/portal/detail/Publication/47985721


Abstract
AT 2018cow was the nearest and best-studied example of a new breed of extragalactic, luminous, and rapidly evolving transient. Both the progenitor systems and explosion mechanisms of these rapid transients remain a mystery - the energetics, spectral signatures, and time-scales make them challenging to interpret in established classes of supernovae and tidal disruption events. The rich, multiwavelength data set of AT 2018cow has still left several interpretations viable to explain the nature of this event. In this paper, we analyze integral-field spectroscopic data of the host galaxy, CGCG137-068, to compare environmental constraints with leading progenitor models. We find the explosion site of AT 2018cow to be very typical of core-collapse supernovae (known to form from stars with M-ZAMS similar to 8-25 M-circle dot), and infer a young stellar population age at the explosion site of few x 10 Myr, at slightly sub-solar metallicity. When comparing to expectations for exotic intermediate-mass black hole (IMBH) tidal disruption events, we find no evidence for a potential host system of the IMBH. In particular, there are no abrupt changes in metallicity or kinematics in the vicinity of the explosion site, arguing against the presence of a distinct host system. The proximity of AT 2018cow to strong star formation in the host galaxy makes us favour a massive stellar progenitor for this event.

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Last updated on 2024-26-11 at 23:12