A1 Vertaisarvioitu alkuperäisartikkeli tieteellisessä lehdessä
Environmental dependence of Type IIn supernova properties
Tekijät: Moriya Takashi J., Galbany Lluís, Jiménez-Palau Cristina, Anderson Joseph P., Kuncarayakti Hanindyo, Sánchez Sebastián F., Lyman Joseph D., Pessi Thallis, Prieto Jose L., Kochanek Christopher S., Dong Subo, Chen Ping
Kustantaja: EDP SCIENCES S A
Julkaisuvuosi: 2023
Journal: Astronomy and Astrophysics
Lehden akronyymi: ASTRON ASTROPHYS
Artikkelin numero: A20
Vuosikerta: 677
Sivujen määrä: 14
ISSN: 0004-6361
eISSN: 1432-0746
DOI: https://doi.org/10.1051/0004-6361/202346703
Verkko-osoite: https://doi.org/10.1051/0004-6361/202346703
Rinnakkaistallenteen osoite: https://research.utu.fi/converis/portal/detail/Publication/181101721
Type IIn supernovae occur when stellar explosions are surrounded by dense hydrogen-rich circumstellar matter. The dense circumstellar matter is likely formed by extreme mass loss from their progenitors shortly before they explode. The nature of Type IIn supernova progenitors and the mass-loss mechanism forming the dense circumstellar matter are still unknown. In this work, we investigate whether Type IIn supernova properties and their local environments are correlated. We use Type IIn supernovae with well-observed light curves and host-galaxy integral field spectroscopic data so that we can estimate both supernova and environmental properties. We find that Type IIn supernovae with a higher peak luminosity tend to occur in environments with lower metallicity and/or younger stellar populations. The circumstellar matter density around Type IIn supernovae is not significantly correlated with metallicity, so the mass-loss mechanism forming the dense circumstellar matter around Type IIn supernovae might be insensitive to metallicity.
Ladattava julkaisu This is an electronic reprint of the original article. |  |
