A1 Vertaisarvioitu alkuperäisartikkeli tieteellisessä lehdessä
JWST and Ground-based Observations of the Type Iax Supernovae SN 2024pxl and SN 2024vjm: Evidence for Weak Deflagration Explosions
Tekijät: Kwok, Lindsey A.; Singh, Mridweeka; Jha, Saurabh W.; Blondin, Stephane; Dastidar, Raya; Larison, Conor; Miller, Adam A.; Andrews, Jennifer E.; Andrews, Moira; Anupama, G. C.; Auchettl, Katie; Banhidi, Dominik; Barna, Barnabas; Bostroem, K. Azalee; Brink, Thomas G.; Cartier, Regis; Chen, Ping; Christy, Collin T.; Coulter, David A.; Covarrubias, Sofia; Davis, Kyle W.; Dickinson, Connor B.; Dong, Yize; Farah, Joseph R.; Filippenko, Alexei V.; Floers, Andreas; Foley, Ryan J.; Franz, Noah; Fremling, Christoffer; Galbany, Lluis; Gangopadhyay, Anjasha; Garg, Aarna; Garnavich, Peter; Gates, Elinor L.; Graur, Or; Gordon, Alexa C.; Hiramatsu, Daichi; Hoang, Emily; Howell, D. Andrew; Hsu, Brian; Johansson, Joel; Joshi, Arti; Kahinga, Lordrick A.; Kaur, Ravjit; Kumar, Sahana; Kumnurdmanee, Piramon; Kuncarayakti, Hanindyo; LeBaron, Natalie; Liu, Chang; Maeda, Keiichi; Maguire, Kate; McCully, Curtis; Mehta, Darshana; Menotti, Luca M.; Metevier, Anne J.; Misra, Kuntal; Murphey, C. Tanner; Newsome, Megan; Padilla Gonzalez, Estefania; Patra, Kishore C.; Pearson, Jeniveve; Piro, Anthony L.; Polin, Abigail; Ravi, Aravind P.; Rest, Armin; Rehemtulla, Nabeel; Meza Retamal, Nicolas; Robinson, Olivia M.; Rojas-Bravo, Cesar; Sahu, Devendra K.; Sand, David J.; Schmidt, Brian P.; Schulze, Steve; Schwab, Michaela; Shrestha, Manisha; Siebert, Matthew R.; Simha, Sunil; Smith, Nathan; Sollerman, Jesper; Subrayan, Bhagya M.; Szalai, Tamas; Taggart, Kirsty; Teja, Rishabh Singh; Temim, Tea; Terwel, Jacco H.; Tinyanont, Samaporn; Valenti, Stefano; Anais Vilchez, Jorge; Vinko, Jozsef; Westerling, Aya L.; Yang, Yi; Zheng, Weikang
Kustantaja: IOP Publishing Ltd
Kustannuspaikka: BRISTOL
Julkaisuvuosi: 2025
Journal: Astrophysical Journal Letters
Tietokannassa oleva lehden nimi: ASTROPHYSICAL JOURNAL LETTERS
Lehden akronyymi: ASTROPHYS J LETT
Artikkelin numero: L33
Vuosikerta: 989
Numero: 2
Sivujen määrä: 24
ISSN: 2041-8205
eISSN: 2041-8213
DOI: https://doi.org/10.3847/2041-8213/adf062
Verkko-osoite: https://iopscience.iop.org/article/10.3847/2041-8213/adf062
Rinnakkaistallenteen osoite: https://research.utu.fi/converis/portal/detail/Publication/499740535
We present panchromatic optical + near-infrared (NIR) + mid-infrared (MIR) observations of the intermediate-luminosity Type Iax supernova (SN Iax) 2024pxl and the extremely low-luminosity SN Iax 2024vjm. JWST observations provide unprecedented MIR spectroscopy of SN Iax, spanning from +11 to +42 day past maximum light. We detect forbidden emission lines in the MIR at these early times while the optical and NIR are dominated by permitted lines with an absorption component. Panchromatic spectra at early times can thus simultaneously show nebular and photospheric lines, probing both inner and outer layers of the ejecta. We identify spectral lines not seen before in SN Iax, including [Mg ii] 4.76 mu m, [Mg ii] 9.71 mu m, [Ne ii] 12.81 mu m, and isolated O i 2.76 mu m that traces unburned material. Forbidden emission lines of all species are centrally peaked with similar kinematic distributions, indicating that the ejecta are well mixed in both SN 2024pxl and SN 2024vjm, a hallmark of pure deflagration explosion models. Radiative transfer modeling of SN 2024pxl shows good agreement with a weak deflagration of a near-Chandrasekhar-mass white dwarf, but additional IR flux is needed to match the observations, potentially attributable to a surviving remnant. Similarly, we find SN 2024vjm is also best explained by a weak deflagration model, despite the large difference in luminosity between the two supernovae. Future modeling should push to even weaker explosions and include the contribution of a bound remnant. Our observations demonstrate the diagnostic power of panchromatic spectroscopy for unveiling explosion physics in thermonuclear supernovae.
Ladattava julkaisu This is an electronic reprint of the original article. |  |
Julkaisussa olevat rahoitustiedot:
https://iopscience.iop.org/article/10.3847/2041-8213/adf062#Acknowledgments
