SN 2019hnl: A Type IIP Supernova with a Partially Stripped, Low-mass Progenitor

Abstract We present optical photometry and spectroscopy of SN 2019hnl. Discovered within ∼26 hr of explosion by the ATLAS survey, SN 2019hnl is a typical Type IIP supernova (SN) with a peak absolute V -band magnitude of −16.7 ± 0.1 mag, a plateau length of ∼107 days, and an early decline rate of 0.0086 ± 0.0006 mag (50 days) −1 . We use nebular spectroscopy and hydrodynamic modeling with the snec , mesa , and stella codes to infer that the progenitor of SN 2019hnl was an M ZAMS ∼ 11 M ⊙ red supergiant, which produced 0.047 ± 0.007 M ⊙ of 56 Ni in the explosion. As a part of our hydrodynamic modeling, we reduced hydrogen envelope mass by scaling the mass loss within the “Dutch” wind scheme to fit our light curve, showing that the progenitor of a relatively typical Type IIP SN may experience partial stripping during their evolution and establish massive (∼0.2 M ⊙ ) circumstellar material environments prior to core collapse.

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Publication Details

Journal
The Astrophysical Journal
Published
2025-10-22
DOI
https://doi.org/10.3847/1538-4357/ae0617
Primary Topic
Gamma-ray bursts and supernovae
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article
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article

SN 2019hnl: A Type IIP Supernova with a Partially Stripped, Low-mass Progenitor

M. Lundquist, Daryl Janzen, Saurabh W. Jha, C. Pellegrino et al.
The Astrophysical Journal
Gamma-ray bursts and supernovae
article

SN 2019hnl: A Type IIP Supernova with a Partially Stripped, Low-mass Progenitor

M. Lundquist, Daryl Janzen, Saurabh W. Jha, C. Pellegrino, Jeniveve Pearson, Aravind P. Ravi, Jennifer E. Andrews, D. Hiramatsu, G. Hosseinzadeh, Yize Dong, Emily Hoang, S. Valenti, David J. Sand, Darshana Mehta, N. Meza, C. McCully, D. A. Howell, Manisha Shrestha, Aidan Martas, K. Azalee Bostroem
article en

Abstract

Abstract We present optical photometry and spectroscopy of SN 2019hnl. Discovered within ∼26 hr of explosion by the ATLAS survey, SN 2019hnl is a typical Type IIP supernova (SN) with a peak absolute V -band magnitude of −16.7 ± 0.1 mag, a plateau length of ∼107 days, and an early decline rate of 0.0086 ± 0.0006 mag (50 days) −1 . We use nebular spectroscopy and hydrodynamic modeling with the snec , mesa , and stella codes to infer that the progenitor of SN 2019hnl was an M ZAMS ∼ 11 M ⊙ red supergiant, which produced 0.047 ± 0.007 M ⊙ of 56 Ni in the explosion. As a part of our hydrodynamic modeling, we reduced hydrogen envelope mass by scaling the mass loss within the “Dutch” wind scheme to fit our light curve, showing that the progenitor of a relatively typical Type IIP SN may experience partial stripping during their evolution and establish massive (∼0.2 M ⊙ ) circumstellar material environments prior to core collapse.

The Astrophysical JournalVol. 993(1)
Openalex Percentile: Top 79%
Gamma-ray bursts and supernovae
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