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The Type II-P Supernova 2019mhm and Constraints on its Progenitor System

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The Type II-P Supernova 2019mhm and Constraints on its Progenitor System. / Vazquez, J.; Kilpatrick, C. D.; Dimitriadis, G. et al.
In: The Astrophysical Journal, Vol. 949, No. 2, 75, 01.06.2023.

Research output: Contribution to Journal/Magazine › Journal article › peer-review

Harvard

Vazquez, J, Kilpatrick, CD, Dimitriadis, G, Foley, RJ, Piro, AL, Rest, A & Rojas-Bravo, C 2023, 'The Type II-P Supernova 2019mhm and Constraints on its Progenitor System', The Astrophysical Journal, vol. 949, no. 2, 75. https://doi.org/10.3847/1538-4357/acbd32

APA

Vazquez, J., Kilpatrick, C. D., Dimitriadis, G., Foley, R. J., Piro, A. L., Rest, A., & Rojas-Bravo, C. (2023). The Type II-P Supernova 2019mhm and Constraints on its Progenitor System. The Astrophysical Journal, 949(2), Article 75. https://doi.org/10.3847/1538-4357/acbd32

Vancouver

Vazquez J, Kilpatrick CD, Dimitriadis G, Foley RJ, Piro AL, Rest A et al. The Type II-P Supernova 2019mhm and Constraints on its Progenitor System. The Astrophysical Journal. 2023 Jun 1;949(2):75. doi: 10.3847/1538-4357/acbd32

Author

Vazquez, J. ; Kilpatrick, C. D. ; Dimitriadis, G. et al. / The Type II-P Supernova 2019mhm and Constraints on its Progenitor System. In: The Astrophysical Journal. 2023 ; Vol. 949, No. 2.

Bibtex

@article{76a8ca965f814621a65d9aef317842ad,
title = "The Type II-P Supernova 2019mhm and Constraints on its Progenitor System",
abstract = "We present pre- and postexplosion observations of the Type II-P supernova (SN II-P) 2019mhm located in NGC 6753. Based on optical spectroscopy and photometry, we show that SN 2019mhm exhibits broad lines of hydrogen with a velocity of −8500 ± 200 km s −1 and a 111 ± 2 day extended plateau in its luminosity, typical of the Type II-P subclass. We also fit its late-time bolometric light curve and infer that it initially produced a 56Ni mass of 1.3 × 10 −2 ± 5.5 × 10 −4 M ⊙. Using imaging from the Wide Field Planetary Camera 2 on the Hubble Space Telescope obtained 19 yr before explosion, we aligned to a postexplosion Wide Field Camera 3 image and demonstrate that there is no detected counterpart to the SN to a limit of >24.53 mag in F814W, corresponding to an absolute magnitude limit of M F814W < −7.7 mag. Comparing to massive-star evolutionary tracks, we determine that the progenitor star had a maximum zero-age main-sequence mass <17.5 M ⊙, consistent with other SN II-P progenitor stars. SN 2019mhm can be added to the growing population of SNe II-P with both direct constraints on the brightness of their progenitor stars and well-observed SN properties.",
author = "J. Vazquez and Kilpatrick, {C. D.} and G. Dimitriadis and Foley, {R. J.} and Piro, {A. L.} and A. Rest and C. Rojas-Bravo",
year = "2023",
month = jun,
day = "1",
doi = "10.3847/1538-4357/acbd32",
language = "English",
volume = "949",
journal = "The Astrophysical Journal",
issn = "0004-637X",
publisher = "Institute of Physics Publishing",
number = "2",

}

RIS

TY - JOUR

T1 - The Type II-P Supernova 2019mhm and Constraints on its Progenitor System

AU - Vazquez, J.

AU - Kilpatrick, C. D.

AU - Dimitriadis, G.

AU - Foley, R. J.

AU - Piro, A. L.

AU - Rest, A.

AU - Rojas-Bravo, C.

PY - 2023/6/1

Y1 - 2023/6/1

N2 - We present pre- and postexplosion observations of the Type II-P supernova (SN II-P) 2019mhm located in NGC 6753. Based on optical spectroscopy and photometry, we show that SN 2019mhm exhibits broad lines of hydrogen with a velocity of −8500 ± 200 km s −1 and a 111 ± 2 day extended plateau in its luminosity, typical of the Type II-P subclass. We also fit its late-time bolometric light curve and infer that it initially produced a 56Ni mass of 1.3 × 10 −2 ± 5.5 × 10 −4 M ⊙. Using imaging from the Wide Field Planetary Camera 2 on the Hubble Space Telescope obtained 19 yr before explosion, we aligned to a postexplosion Wide Field Camera 3 image and demonstrate that there is no detected counterpart to the SN to a limit of >24.53 mag in F814W, corresponding to an absolute magnitude limit of M F814W < −7.7 mag. Comparing to massive-star evolutionary tracks, we determine that the progenitor star had a maximum zero-age main-sequence mass <17.5 M ⊙, consistent with other SN II-P progenitor stars. SN 2019mhm can be added to the growing population of SNe II-P with both direct constraints on the brightness of their progenitor stars and well-observed SN properties.

AB - We present pre- and postexplosion observations of the Type II-P supernova (SN II-P) 2019mhm located in NGC 6753. Based on optical spectroscopy and photometry, we show that SN 2019mhm exhibits broad lines of hydrogen with a velocity of −8500 ± 200 km s −1 and a 111 ± 2 day extended plateau in its luminosity, typical of the Type II-P subclass. We also fit its late-time bolometric light curve and infer that it initially produced a 56Ni mass of 1.3 × 10 −2 ± 5.5 × 10 −4 M ⊙. Using imaging from the Wide Field Planetary Camera 2 on the Hubble Space Telescope obtained 19 yr before explosion, we aligned to a postexplosion Wide Field Camera 3 image and demonstrate that there is no detected counterpart to the SN to a limit of >24.53 mag in F814W, corresponding to an absolute magnitude limit of M F814W < −7.7 mag. Comparing to massive-star evolutionary tracks, we determine that the progenitor star had a maximum zero-age main-sequence mass <17.5 M ⊙, consistent with other SN II-P progenitor stars. SN 2019mhm can be added to the growing population of SNe II-P with both direct constraints on the brightness of their progenitor stars and well-observed SN properties.

U2 - 10.3847/1538-4357/acbd32

DO - 10.3847/1538-4357/acbd32

M3 - Journal article

VL - 949

JO - The Astrophysical Journal

JF - The Astrophysical Journal

SN - 0004-637X

IS - 2

M1 - 75

ER -