Abstract
We consider the effect of a change in the rate of flux decline in the \(U\) band for type II-P supernovae (SNe IIP) as a function of metallicity \(Z\). Based on this effect, we propose a new method to determine the photometric redshift from the SN IIP light curve in the \(U\) band. Using the STELLA code, we have constructed model light curves in different bands for different redshifts \(z=0.0\), 0.1, and 0.3 as the metallicity in the models decreases from \(Z\sim 10^{-3}\) to \({\sim}10^{-6}\). The flux in the \(U\) band is shown to reach a plateau at the lowest metallicities. We consider the influence of other parameters as well: the presupernova mass and the mass of radioactive nickel-56.
This is a preview of subscription content, log in via an institution to check access.
Similar content being viewed by others
REFERENCES
P. V. Baklanov, S. I. Blinnikov, and N. N. Pavlyuk, Astron. Lett. 31, 429 (2005).
S. I. Blinnikov and E. I. Sorokina, Astron. Astrophys. 356, L30 (2000).
S. I. Blinnikov, F. K. Röpke, E. I. Sorokina, M. Gieseler, M. Reinecke, C. Travaglio, W. Hillebrandt, and M. Stritzinge, Astron. Astrophys. 453, 229 (2006).
S. Bose, S. Dong, C. S. Kochanek, A. Pastorello, B. Katz, D. Bersier, J. E. Andrews, J. L. Prieto, et al., Astrophys. J. 862, 107 (2018).
L. Dessart D. J. Hillier, R. Waldman, and E. Livne, Mon. Not. R. Astron. Soc. 433, 1745 (2013).
R. G. Eastman S. E. Woosley, T. A. Weaver, and P. A. Pinto, Astrophys. J. 430, 300 (1994).
T. Faran, D. Poznanski, A. V. Filippenko, et al., Mon. Not. R. Astron. Soc. 445, 554 (2014).
M. Hicken, A. S. Friedman, S. Blondin, P. Challis, P. Berlind, M. Calkins, G. Esquerdo, Th. Matheson, et al., Astrophys. J. Suppl. Ser. 233, 6 (2017).
V. S. Imshennik and D. K. Nadyozhin, Sov. Sci. Rev., Sect. E 8, 1 (1989).
R. Kessler et al., Astrophys. J. 717, 40 (2010).
D. C. Koo, Astron. J. 90, 418 (1985).
D. C. Leonard, A. V. Filippenko, W. Li, et al., Publ. Astron. Soc. Pacif. 114, 35 (2002).
LSST Science Collab., 247 colleagues, arXiv:0912.0201 (2009).
V. Morozova et al., Astrophys. J. 814, 83 (2015).
T. Nordlander, M. S. Bessell, G. S. Da Costa, et al., Mon. Not. R. Astron. Soc. 488, L109 (2019).
N. Padmanabhan, T. Bu-davari, D. J. Schlegel, et al., Mon. Not. R. Astron. Soc. 359, 237 (2005).
N. Palanque-Delabrouille, V. Ruhlmann-Kleider, S. Pascal, J. Rich, J. Guy, G. Bazin, P. Astier, C. Balland, et al., Astron. Astrophys. 514, A63 (2010).
M. Potashov and A. Yudin, Mon. Not. R. Astron. Soc. 491, 2674 (2020).
A. Tolstov, K. Nomoto, N. Tominaga, M. N. Ishigaki, S. Blinnikov, and T. Suzuki, Astrophys. J. 821, 124 (2016).
V. P. Utrobin, Astron. Astrophys. 461, 233 (2007).
V. P. Utrobin and N. N. Chugai, Astron. Lett. 28, 386 (2002).
V. P. Utrobin and N. N. Chugai, Astron. Astrophys. 441, 271 (2005).
Y. Wang, Astrophys. J. Lett. 654, L123 (2007).
Y. Wang, E. Gjergo, and S. Kuhlmann, Mon. Not. R. Astron. Soc. 451, 1955 (2015).
ACKNOWLEDGMENTS
A.A. Goldshtein thanks P.V. Baklanov and M.Sh. Potashov for their help in preparing this paper and M.V. Kostina for the useful discussions. S.I. Blinnikov thanks the Russian Science Foundation for its support of the work on the development of the STELLA code (project no. 19-12-00229).
Author information
Authors and Affiliations
Corresponding authors
Additional information
Translated by V. Astakhov
Rights and permissions
About this article
Cite this article
Goldshtein, A.A., Blinnikov, S.I. Study of the Dependence of the Plateau Shape for Type II Supernovae on Metallicity. Astron. Lett. 46, 312–318 (2020). https://doi.org/10.1134/S1063773720050047
Received:
Revised:
Accepted:
Published:
Issue Date:
DOI: https://doi.org/10.1134/S1063773720050047