Constraints on core-collapse supernova progenitors from explosion site integral field spectroscopy
Abstract
Observationally, supernovae (SNe) are divided into subclasses according to their distinct characteristics. This diversity naturally reflects the diversity in the progenitor stars. It is not entirely clear, however, how different evolutionary paths leading massive stars to become an SN are governed by fundamental parameters such as progenitor initial mass and metallicity. Furthermore, this paper places constraints on progenitor initial mass and metallicity in distinct core-collapse SN subclasses through a study of the parent stellar populations at the explosion sites. Integral field spectroscopy (IFS) of 83 nearby SN explosion sites with a median distance of 18 Mpc has been collected and analysed, enabling detection and spectral extraction of the parent stellar population of SN progenitors. From the parent stellar population spectrum, the initial mass and metallicity of the coeval progenitor are derived by means of comparison to simple stellar population models and strong-line methods. Additionally, near-infrared IFS was employed to characterise the star formation history at the explosion sites. No significant metallicity differences are observed among distinct SN types. The typical progenitor mass is found to be highest for SN type Ic, followed by type Ib, then types IIb and II. Type IIn is the least associated with young stellar populationsmore »
- Authors:
-
[1];
- Univ. of Turku, Piikkiö (Finland); Millennium Inst. of Astrophysics, Santiago (Chile); Univ. de Chile, Santiago (Chile)
- European Southern Observatory, Santiago (Chile)
- Univ. of Pittsburgh, Pittsburgh, PA (United States)
- Kyoto Univ., Kyoto (Japan); The Univ. of Tokyo, Chiba (Japan)
- Millennium Inst. of Astrophysics, Santiago (Chile); Univ. de Chile, Santiago (Chile)
- Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
- Seoul National Univ., Seoul (Korea); National Institutes of Natural Sciences, Hilo, HI (United States)
- Univ. of Tokyo, Tokyo (Japan)
- National Astronomical Observatory of Japan, Tokyo (Japan); SOKENDAI (The Graduate Univ. for Advanced Studies), Tokyo (Japan)
- Publication Date:
- Research Org.:
- Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States). National Energy Research Scientific Computing Center (NERSC)
- Sponsoring Org.:
- USDOE
- OSTI Identifier:
- 1543824
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Astronomy and Astrophysics
- Additional Journal Information:
- Journal Volume: 613; Journal ID: ISSN 0004-6361
- Publisher:
- EDP Sciences
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; Astronomy & Astrophysics; supernovae: general; stars: massive
Citation Formats
Kuncarayakti, Hanindyo, Anderson, J. P., Galbany, L., Maeda, K., Hamuy, M., Aldering, G., Arimoto, N., Doi, M., Morokuma, T., and Usuda, T. Constraints on core-collapse supernova progenitors from explosion site integral field spectroscopy. United States: N. p., 2018.
Web. doi:10.1051/0004-6361/201731923.
Kuncarayakti, Hanindyo, Anderson, J. P., Galbany, L., Maeda, K., Hamuy, M., Aldering, G., Arimoto, N., Doi, M., Morokuma, T., & Usuda, T. Constraints on core-collapse supernova progenitors from explosion site integral field spectroscopy. United States. https://doi.org/10.1051/0004-6361/201731923
Kuncarayakti, Hanindyo, Anderson, J. P., Galbany, L., Maeda, K., Hamuy, M., Aldering, G., Arimoto, N., Doi, M., Morokuma, T., and Usuda, T. Mon .
"Constraints on core-collapse supernova progenitors from explosion site integral field spectroscopy". United States. https://doi.org/10.1051/0004-6361/201731923. https://www.osti.gov/servlets/purl/1543824.
@article{osti_1543824,
title = {Constraints on core-collapse supernova progenitors from explosion site integral field spectroscopy},
author = {Kuncarayakti, Hanindyo and Anderson, J. P. and Galbany, L. and Maeda, K. and Hamuy, M. and Aldering, G. and Arimoto, N. and Doi, M. and Morokuma, T. and Usuda, T.},
abstractNote = {Observationally, supernovae (SNe) are divided into subclasses according to their distinct characteristics. This diversity naturally reflects the diversity in the progenitor stars. It is not entirely clear, however, how different evolutionary paths leading massive stars to become an SN are governed by fundamental parameters such as progenitor initial mass and metallicity. Furthermore, this paper places constraints on progenitor initial mass and metallicity in distinct core-collapse SN subclasses through a study of the parent stellar populations at the explosion sites. Integral field spectroscopy (IFS) of 83 nearby SN explosion sites with a median distance of 18 Mpc has been collected and analysed, enabling detection and spectral extraction of the parent stellar population of SN progenitors. From the parent stellar population spectrum, the initial mass and metallicity of the coeval progenitor are derived by means of comparison to simple stellar population models and strong-line methods. Additionally, near-infrared IFS was employed to characterise the star formation history at the explosion sites. No significant metallicity differences are observed among distinct SN types. The typical progenitor mass is found to be highest for SN type Ic, followed by type Ib, then types IIb and II. Type IIn is the least associated with young stellar populations and thus massive progenitors. However, statistically significant differences in progenitor initial mass are observed only when comparing SNe IIn with other subclasses. Stripped-envelope SN progenitors with initial mass estimates lower than 25 M⊙ are found; they are thought to be the result of binary progenitors. Confirming previous studies, these results support the notion that core-collapse SN progenitors cannot arise from single-star channels only, and both single and binary channels are at play in the production of core-collapse SNe. Near-infrared IFS suggests that multiple stellar populations with different ages may be present in some of the SN sites. As a consequence, there could be a non-negligible amount of contamination from old populations, and therefore the individual age estimates are effectively lower limits.},
doi = {10.1051/0004-6361/201731923},
journal = {Astronomy and Astrophysics},
number = ,
volume = 613,
place = {United States},
year = {Mon May 28 00:00:00 EDT 2018},
month = {Mon May 28 00:00:00 EDT 2018}
}
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Figures / Tables:
Fig. 1: Relative frequency of each SN type in the current sample (large pie chart), compared to that of LOSS (Smith et al. 2011a, small pie chart in pale colours).
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A hybrid envelope-stripping mechanism for massive stars from supernova nebular spectroscopy
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- Fang, Qiliang; Maeda, Keiichi; Kuncarayakti, Hanindyo
- Nature Astronomy, Vol. 3, Issue 5
Relativistic supernova 2009bb exploded close to an atomic gas cloud
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The extraplanar type II supernova ASASSN-14jb in the nearby edge-on galaxy ESO 467-G051
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A meta-analysis of core-collapse supernova 56 Ni masses
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The diverse lives of progenitors of hydrogen-rich core-collapse supernovae: the role of binary interaction
journal, October 2019
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Core-collapse supernovae ages and metallicities from emission-line diagnostics of nearby stellar populations
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Investigating the properties of stripped-envelope supernovae; what are the implications for their progenitors?
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- Monthly Notices of the Royal Astronomical Society, Vol. 485, Issue 2
The 50–100 pc scale parent stellar populations of Type II supernovae and limitations of single star evolution models
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The radial distribution of supernovae compared to star formation tracers
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A Long-duration Luminous Type IIn Supernova KISS15s: Strong Recombination Lines from the Inhomogeneous Ejecta–CSM Interaction Region and Hot Dust Emission from Newly Formed Dust
journal, February 2019
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Core-collapse supernovae ages and metallicities from emission-line diagnostics of nearby stellar populations
text, January 2018
- Xiao, Lin; Galbany, L.; Eldridge, J. J.
- arXiv
Relativistic supernova 2009bb exploded close to an atomic gas cloud
text, January 2018
- Michałowski, Michał J.; Gentile, G.; Kruhler, T.
- arXiv
Investigating the properties of stripped-envelope supernovae, what are the implications for their progenitors?
text, January 2018
- Prentice, S. J.; Ashall, C.; James, P. A.
- arXiv
The radial distribution of supernovae compared to star formation tracers
text, January 2019
- Audcent-Ross, Fiona M.; Meurer, Gerhardt R.; Audcent, James R.
- arXiv
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