JWST and Ground-based Observations of the Type Iax Supernovae SN 2024pxl and SN 2024vjm: Evidence for Weak Deflagration Explosions
Abstrak
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 μ m, [Mg ii ] 9.71 μ m, [Ne ii ] 12.81 μ m, and isolated O i 2.76 μ 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.
Topik & Kata Kunci
Penulis (92)
Lindsey A. Kwok
Mridweeka Singh
Saurabh W. Jha
Stéphane Blondin
Raya Dastidar
Conor Larison
Adam A. Miller
Jennifer E. Andrews
Moira Andrews
G. C. Anupama
Katie Auchettl
Dominik Bánhidi
Barnabas Barna
K. Azalee Bostroem
Thomas G. Brink
Régis Cartier
Ping Chen
Collin T. Christy
David A. Coulter
Sofia Covarrubias
Kyle W. Davis
Connor B. Dickinson
Yize Dong
Joseph R. Farah
Alexei V. Filippenko
Andreas Flörs
Ryan J. Foley
Noah Franz
Christoffer Fremling
Lluís Galbany
Anjasha Gangopadhyay
Aarna Garg
Peter Garnavich
Elinor L. Gates
Or Graur
Alexa C. Gordon
Daichi Hiramatsu
Emily Hoang
D. Andrew Howell
Brian Hsu
Joel Johansson
Arti Joshi
Lordrick A. Kahinga
Ravjit Kaur
Sahana Kumar
Piramon Kumnurdmanee
Hanindyo Kuncarayakti
Natalie LeBaron
Chang Liu
Keiichi Maeda
Kate Maguire
Curtis McCully
Darshana Mehta
Luca M. Menotti
Anne J. Metevier
Kuntal Misra
C. Tanner Murphey
Megan Newsome
Estefania Padilla Gonzalez
Kishore C. Patra
Jeniveve Pearson
Anthony L. Piro
Abigail Polin
Aravind P. Ravi
Armin Rest
Nabeel Rehemtulla
Nicolas Meza Retamal
Olivia M. Robinson
César Rojas-Bravo
Devendra K. Sahu
David J. Sand
Brian P. Schmidt
Steve Schulze
Michaela Schwab
Manisha Shrestha
Matthew R. Siebert
Sunil Simha
Nathan Smith
Jesper Sollerman
Bhagya M. Subrayan
Tamás Szalai
Kirsty Taggart
Rishabh Singh Teja
Tea Temim
Jacco H. Terwel
Samaporn Tinyanont
Stefano Valenti
Jorge Anais Vilchez
József Vinkó
Aya L. Westerling
Yi Yang
WeiKang Zheng
Akses Cepat
- Tahun Terbit
- 2025
- Sumber Database
- DOAJ
- DOI
- 10.3847/2041-8213/adf062
- Akses
- Open Access ✓