Core-Collapse Supernova Subtypes in Luminous Infrared Galaxies
Astronomy & Astrophysics manuscript no. aa ©ESO 2021 March 1, 2021 Core-collapse supernova subtypes in luminous infrared galaxies E. Kankare1, A. Efstathiou2, R. Kotak1, E. C. Kool3, T. Kangas4, D. O’Neill5, S. Mattila1, P. Väisänen6, 7, R. Ramphul6, 8, M. Mogotsi6, S. D. Ryder9, 10, S. Parker11, 12, T. Reynolds1, M. Fraser13, A. Pastorello14, E. Cappellaro14, P. A. Mazzali15, 16, P. Ochner17, 14, L. Tomasella14, M. Turatto14, J. Kotilainen18, 1, H. Kuncarayakti1, 18, M. A. Pérez-Torres19, 20, Z. Randriamanakoto6 , C. Romero-Cañizales21, M. Berton18, 22, R. Cartier23, T.-W. Chen3, L. Galbany24, M. Gromadzki25, C. Inserra26, K. Maguire27, S. Moran1, T. E. Müller-Bravo28, M. Nicholl29, 30, A. Reguitti13, 31, 32, and D. R. Young5 (Affiliations can be found after the references) March 1, 2021 ABSTRACT The fraction of core-collapse supernovae (CCSNe) occurring in the central regions of galaxies is not well-constrained at present. This is partly because large-scale transient surveys operate at optical wavelengths, making it challenging to detect transient sources that occur in regions suscep- tible to high extinction factors. Here we present the discovery and follow-up observations of two CCSNe that occurred in the luminous infrared galaxy (LIRG), NGC 3256. The first, SN 2018ec, was discovered using the ESO HAWK-I/GRAAL adaptive optics seeing enhancer, and was +0.3 classified as a Type Ic with a host galaxy extinction of AV = 2.1−0.1 mag. The second, AT 2018cux, was discovered during the course of follow-up observations of SN 2018ec, and is consistent with a sub-luminous Type IIP classification with an AV = 2.1 ± 0.4 mag of host extinction.
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