Reguitti, A ORCID: 0000-0003-4254-2724, Pastorello, A
ORCID: 0000-0002-7259-4624, Pignata, G, Fraser, M
ORCID: 0000-0003-2191-1674, Stritzinger, MD
ORCID: 0000-0002-5571-1833, Brennan, SJ, Cai, YZ
ORCID: 0000-0002-7714-493X, Elias-Rosa, N
ORCID: 0000-0002-1381-9125, Fugazza, D, Gutierrez, CP
ORCID: 0000-0003-2375-2064, Kankare, E, Kotak, R, Lundqvist, P, Mazzali, PA
ORCID: 0000-0001-6876-8284, Moran, S, Salmaso, I, Tomasella, L
ORCID: 0000-0002-3697-2616, Valerin, G and Kuncarayakti, H
(2022)
SN 2021foa, a transitional event between a Type IIn (SN 2009ip-like) and a Type Ibn supernova.
Astronomy and Astrophysics, 662.
ISSN 0004-6361
Preview |
Text
SN 2021foa a transitional event between a Type IIn (SN 2009ip-like) and a Typle Ibn supernova.pdf - Published Version Available under License Creative Commons Attribution. Download (1MB) | Preview |
Abstract
We present photometric and spectroscopic data of the unusual interacting supernova (SN) 2021foa. It rose to an absolute magnitude peak of Mr= 18 mag in 20 days. The initial light curve decline shows some luminosity fluctuations before a long-lasting flattening. A faint source (Mr∼ 14 mag) was detected in the weeks preceding the main event, showing a slowly rising luminosity trend. The r-band absolute light curve is very similar to those of SN 2009ip-like events, with a faint and shorter duration brightening ('Event A') followed by a much brighter peak ('Event B'). The early spectra of SN 2021foa show a blue continuum with narrow (∼400 km s1) H emission lines that, two weeks later, reveal a complex profile, with a narrow P Cygni on top of an intermediate-width (∼2700 km s1) component. At +12 days, metal lines in emission appear and Hea lines become very strong, with Hea λ5876 reaching half of the Hα luminosity, much higher than in previous SN 2009ip-like objects. We propose that SN 2021foa is a transitional event between the H-rich SN 2009ip-like SNe and the He-rich Type Ibn SNe.
Item Type: | Article |
---|---|
Uncontrolled Keywords: | 0201 Astronomical and Space Sciences; Astronomy & Astrophysics |
Subjects: | Q Science > QB Astronomy |
Divisions: | Astrophysics Research Institute |
Publisher: | EDP Sciences |
Date of acceptance: | 5 June 2022 |
Date of first compliant Open Access: | 1 November 2022 |
Date Deposited: | 01 Nov 2022 16:59 |
Last Modified: | 05 Jul 2025 12:45 |
DOI or ID number: | 10.1051/0004-6361/202243340 |
URI: | https://researchonline.ljmu.ac.uk/id/eprint/17997 |
![]() |
View Item |