The bolometric light curves and physical parameters of stripped-envelope supernovae
Abstract
The optical and optical/near-infrared pseudo-bolometric light curves of 85 stripped-envelope supernovae (SNe) are constructed using a consistent method and a standard cosmology. The light curves are analysed to derive temporal characteristics and peak luminosity Lp , enabling the construction of a luminosity function. Subsequently, the mass of 56 Ni synthesized in the explosion, along with the ratio of ejecta mass to ejecta kinetic energy, are found. Analysis shows that host-galaxy extinction is an important factor in accurately determining luminosity values as it is significantly greater than Galactic extinction in most cases. It is found that broad-lined SNe Ic (SNe Ic-BL) and gamma-ray burst SNe are the most luminous subtypes with a combined median Lp , in erg s-1 , of log(Lp) = 43.00 compared to 42.51 for SNe Ic, 42.50 for SNe Ib, and 42.36 for SNe IIb. It is also found that SNe Ic-BL synthesize approximately twice the amount of 56Ni compared with SNe Ic, Ib, and IIb, with median MNi = 0.34, 0.16, 0.14, and 0.11 M ⊙ , respectively. SNe Ic-BL, and to a lesser extent SNe Ic, typically rise from L p /2 to L p more quickly than SNe Ib/IIb; consequently, their light curves aremore »
- Authors:
-
- Liverpool John Moores Univ. (United Kingdom)
- Liverpool John Moores Univ. (United Kingdom); Max Planck Society, Garching (Germany). Max Planck Inst. for Astrophysik
- Inst. of Space Astrophyics and Cosmic Physics, Bologna (Italy); Scuola Normale Superiore (SNS), Pisa (Italy)
- Weizmann Inst. of Science, Rehovot (Israel)
- California Inst. of Technology (CalTech), Pasadena, CA (United States)
- Texas Tech Univ., Lubbock, TX (United States)
- Stockholm Univ. (Sweden)
- Univ. of California, Santa Barbara, CA (United States). Kavli Inst. for Theoretical Physics; 9Las Cumbres Observatory Global Telescope Network, Goleta, CA (United States)
- Univ. of California, Berkeley, CA (United States)
- California Inst. of Technology (CalTech), Pasadena, CA (United States); Carnegie Inst. of Science, Pasadena, CA (United States)
- NASA Goddard Space Flight Center (GSFC), Greenbelt, MD (United States)
- Univ. of California, Berkeley, CA (United States); Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
- Publication Date:
- Research Org.:
- Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC)
- OSTI Identifier:
- 1393035
- Grant/Contract Number:
- AC02-05CH11231
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Monthly Notices of the Royal Astronomical Society
- Additional Journal Information:
- Journal Volume: 458; Journal Issue: 3; Journal ID: ISSN 0035-8711
- Publisher:
- Royal Astronomical Society
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS
Citation Formats
Prentice, S. J., Mazzali, P. A., Pian, E., Gal-Yam, A., Kulkarni, S. R., Rubin, A., Corsi, A., Fremling, C., Sollerman, J., Yaron, O., Arcavi, I., Zheng, W., Kasliwal, M. M., Filippenko, A. V., Cenko, S. B., Cao, Y., and Nugent, P. E. The bolometric light curves and physical parameters of stripped-envelope supernovae. United States: N. p., 2016.
Web. doi:10.1093/mnras/stw299.
Prentice, S. J., Mazzali, P. A., Pian, E., Gal-Yam, A., Kulkarni, S. R., Rubin, A., Corsi, A., Fremling, C., Sollerman, J., Yaron, O., Arcavi, I., Zheng, W., Kasliwal, M. M., Filippenko, A. V., Cenko, S. B., Cao, Y., & Nugent, P. E. The bolometric light curves and physical parameters of stripped-envelope supernovae. United States. https://doi.org/10.1093/mnras/stw299
Prentice, S. J., Mazzali, P. A., Pian, E., Gal-Yam, A., Kulkarni, S. R., Rubin, A., Corsi, A., Fremling, C., Sollerman, J., Yaron, O., Arcavi, I., Zheng, W., Kasliwal, M. M., Filippenko, A. V., Cenko, S. B., Cao, Y., and Nugent, P. E. Mon .
"The bolometric light curves and physical parameters of stripped-envelope supernovae". United States. https://doi.org/10.1093/mnras/stw299. https://www.osti.gov/servlets/purl/1393035.
@article{osti_1393035,
title = {The bolometric light curves and physical parameters of stripped-envelope supernovae},
author = {Prentice, S. J. and Mazzali, P. A. and Pian, E. and Gal-Yam, A. and Kulkarni, S. R. and Rubin, A. and Corsi, A. and Fremling, C. and Sollerman, J. and Yaron, O. and Arcavi, I. and Zheng, W. and Kasliwal, M. M. and Filippenko, A. V. and Cenko, S. B. and Cao, Y. and Nugent, P. E.},
abstractNote = {The optical and optical/near-infrared pseudo-bolometric light curves of 85 stripped-envelope supernovae (SNe) are constructed using a consistent method and a standard cosmology. The light curves are analysed to derive temporal characteristics and peak luminosity Lp , enabling the construction of a luminosity function. Subsequently, the mass of 56 Ni synthesized in the explosion, along with the ratio of ejecta mass to ejecta kinetic energy, are found. Analysis shows that host-galaxy extinction is an important factor in accurately determining luminosity values as it is significantly greater than Galactic extinction in most cases. It is found that broad-lined SNe Ic (SNe Ic-BL) and gamma-ray burst SNe are the most luminous subtypes with a combined median Lp , in erg s-1 , of log(Lp) = 43.00 compared to 42.51 for SNe Ic, 42.50 for SNe Ib, and 42.36 for SNe IIb. It is also found that SNe Ic-BL synthesize approximately twice the amount of 56Ni compared with SNe Ic, Ib, and IIb, with median MNi = 0.34, 0.16, 0.14, and 0.11 M ⊙ , respectively. SNe Ic-BL, and to a lesser extent SNe Ic, typically rise from L p /2 to L p more quickly than SNe Ib/IIb; consequently, their light curves are not as broad.},
doi = {10.1093/mnras/stw299},
journal = {Monthly Notices of the Royal Astronomical Society},
number = 3,
volume = 458,
place = {United States},
year = {Mon Feb 08 00:00:00 EST 2016},
month = {Mon Feb 08 00:00:00 EST 2016}
}
Web of Science
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Spectra of Hydrogen-Poor Superluminous Supernovae from the Palomar Transient Factory
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Observational properties of a Type Ib Supernova MASTER OT J120451.50+265946.6 in NGC 4080
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