Transitional events in the spectrophotometric regime between stripped envelope and superluminous supernovae
Metadatos
Afficher la notice complèteEditorial
Oxford University Press
Materia
Supernovae General
Date
2021-10-05Referencia bibliográfica
S J Prentice, C Inserra, S Schulze, M Nicholl, P A Mazzali, S D Vergani, L Galbany, J P Anderson, C Ashall, T W Chen, M Deckers, M Delgado Mancheño, R González Díaz, S González-Gaitán, M Gromadzki, C P Gutiérrez, L Harvey, A Kozyreva, M R Magee, K Maguire, T E Müller-Bravo, S Muñoz Torres, P J Pessi, J Sollerman, J Teffs, J H Terwel, D R Young, Transitional events in the spectrophotometric regime between stripped envelope and superluminous supernovae, Monthly Notices of the Royal Astronomical Society, Volume 508, Issue 3, December 2021, Pages 4342–4358, [https://doi.org/10.1093/mnras/stab2864]
Patrocinador
H2020 ERC grant no. 758638; European Union’s Horizon 2020 research and innovation programme under the Marie Skłodowska-Curie grant agreement no. 839090; Spanish Ministry of Science, Innovation and Universities (MICIU) under the 2019 Ramon y Cajal programme RYC2019-027683; CONICYT PFCHA / DOCTORADOBECAS CHILE/2017-72180113; EU Horizon 2020 research and innovation programme under grant agreement no. 101004719; FCT under Project CRISP PTDC/FIS-AST-31546/2017; Royal Astronomical Society Research Fellowship; H2020 ERC grant no. 948381; UK Science and Technology Facilities Council; ESO programme ID 1103.D-0328 (PI: Inserra)Résumé
The division between stripped-envelope supernovae (SE-SNe) and superluminous supernovae (SLSNe) is not well-defined in either photometric or spectroscopic space. While a sharp luminosity threshold has been suggested, there remains an increasing number of transitional objects that reach this threshold without the spectroscopic signatures common to SLSNe. In this work, we present data and analysis on four SNe transitional between SE-SNe and SLSNe; the He-poor SNe 2019dwa and 2019cri, and the He-rich SNe 2019hge and 2019unb. Each object displays long-lived and variable photometric evolution with luminosities around the SLSN threshold of Mr < -19.8 mag. Spectroscopically however, these objects are similar to SE-SNe, with line velocities lower than either SE-SNe and SLSNe, and thus represent an interesting case of rare transitional events.