A1 Refereed original research article in a scientific journal

Red eminence : The intermediate-luminosity red transient AT 2022fnm




AuthorsMoran, S.; Kotak, R.; Fraser, M.; Pastorello, A.; Cai, Y.-Z.; Valerin, G.; Mattila, S.; Cappellaro, E.; Kravtsov, T.; Gutiérrez, C. P.; Elias-Rosa, N.; Reguitti, A.; Lundqvist, P.; Filippenko, A. V.; Brink, T. G.; Wang, X.-F.

PublisherEDP Sciences

Publication year2024

JournalAstronomy and Astrophysics

Journal name in sourceAstronomy & Astrophysics

Article numberA161

Volume688

ISSN0004-6361

eISSN1432-0746

DOIhttps://doi.org/10.1051/0004-6361/202348225

Web address http://dx.doi.org/10.1051/0004-6361/202348225

Self-archived copy’s web addresshttps://research.utu.fi/converis/portal/detail/Publication/457600334

Preprint addresshttps://arxiv.org/abs/2406.02816


Abstract

We present results from a five-month-long observing campaign of the unusual transient AT 2022fnm, which displays properties common to both luminous red novae (LRNe) and intermediate-luminosity red transients (ILRTs). Although its photometric evolution is broadly consistent with that of LRNe, no second peak is apparent in its light curve, and its spectral properties are more reminiscent of ILRTs. It has a fairly rapid rise time of 5.3 ± 1.5 d, reaching a peak absolute magnitude of −12.7 ± 0.1 (in the ATLAS o band). We find some evidence for circumstellar interaction, and a near-infrared excess becomes apparent at approximately +100 d after discovery. We attribute this to a dust echo. Finally, from an analytical diffusion toy model, we attempted to reproduce the pseudo-bolometric light curve and find that a mass of ∼4 M is needed. Overall, the characteristics of AT 2022fnm are consistent with a weak stellar eruption or an explosion reminiscent of low-energy type IIP supernovae, which is compatible with expectations for ILRTs.


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Funding information in the publication
Research funded by Research Council of Finland (340613) | NASA/HST (AR-14295) | National Natural Science Foundation of China (12303054) | International Centre of Supernovae, Yunnan Key Laboratory (202302AN360001) | Academy of Finland (350458) | Marie Skłodowska-Curie and the Beatriu de Pinós (2021 BP 00168) | Ministerio de Ciencia e Innovación (PID2020-115253GA-I00) | Unidad de Excelencia María de Maeztu (CEX2020-001058-M) | PRIN 2017 (20179ZF5KS) | MICINN (PID2019-108709GB-I00) | Beijing Academy of Science and Technology (DZ:BS202002) | National Natural Science Foundation of China (12033003,11633002)


Last updated on 2025-27-01 at 19:59