Abstract
The September 2012 outburst of the type IIn supernova 2009ip was simulated using two independent codes, STELLA and FRONT. The \(UBVRI\) light curves obtained agree well with one another and with observational data. Special attention is given to the dynamics of the emerging dense shell, which determines the luminosity of the object and is used for the direct method of determining the distance to the supernova. Two-dimensional spectral radiation-hydrodynamics computations of the SN 2009ip model were carried out, which confirmed the conclusion about the stability of this shell on the times scales of the method application.
REFERENCES
D. A. Badjin and S. I. Glazyrin, Mon. Not. R. Astron. Soc. 507, 1492 (2021).
D. A. Badjin, S. I. Glazyrin, K. V. Manukovskiy, and S. I. Blinnikov, Mon. Not. R. Astron. Soc. 459, 2188 (2016).
P. V. Baklanov, S. I. Blinnikov, M. Sh. Potashov, and A. D. Dolgov, JETP Lett. 98, 432 (2013).
S. I. Blinnikov, Astron. Lett. 22, 79 (1996).
S. I. Blinnikov, R. Eastman, O. S. Bartunov, V. A. Popolitov, and S. E. Woosley, Astrophys. J. 496, 454 (1998).
S. I. Blinnikov, F. K. Ropke, E. I. Sorokina, M. Gieseler, M. Reinecke, C. Travaglio, W. Hillebrandt, and M. Stritzinger, Astron. Astrophys. 453, 229 (2006).
S. Blinnikov, M. Potashov, P. Baklanov, and A. Dolgov, JETP Lett. 96, 153 (2012).
R. Chevalier and J. M. Blondin, Astrophys. J. 444, 312 (1995).
N. N. Chugai, Astron. Lett. 48, 442 (2022).
B. Dubroca and J.-L. Feugeas, C.R. Acad. Sci., Ser. Math. 329, 915 (1999).
D. B. Friend and J. I. Castor, Astrophys. J. 272, 259 (1983).
A. H. Karp, G. Lasher, K. L. Chan, and E. E. Salpeter, Astrophys. J. 214, 161 (1977).
A. Kashi, N. Soker, and N. Moskovitz, Mon. Not. R. Astron. Soc. 436, 2484 (2013).
C. S. Kochanek, D. M. Szczygieł, and K. Z. Stanek, Astrophys. J. 758, 142 (2012).
A. Kozyreva, L. Shingles, A. Mironov, P. Baklanov, and S. Blinnikov, Mon. Not. R. Astron. Soc. 499, 4312 (2020).
R. L. Kurucz, Rev. Mex. Astron. Astrofis. 23 (1992).
C. Levermore, J. Quant. Spectrosc. Rad. Transfer 31, 149 (1984).
M. S. Liou, J. Comput. Phys. 160, 623 (2000).
R. Margutti, D. Milisavljevic, A. M. Soderberg, R. Chornock, B. A. Zauderer, K. Murase, C. Guidorzi, N. E. Sanders, et al., Astrophys. J. 780, 21 (2014).
J. Maza, M. Hamuy, R. Antezana, L. Gonzalez, P. Lopez, S. Silva, G. Folatelli, D. Iturra, et al., Centr. Bureau Electron. Telegrams 1928, 1 (2009).
A. McDowell, P. Duffell, and D. Kasen, Am. Astron. Soc. Meet. Abstr. 229, 434 (2017).
T. J. Moriya, S. I. Blinnikov, N. Tominaga, N. Yoshida, M. Tanaka, K. Maeda, and K. Nomoto, Mon. Not. R. Astron. Soc. 428, 1020 (2013).
A. Pastorello, E. Cappellaro, C. Inserra, S. J. Smartt, G. Pignata, S. Benetti, S. Valenti, M. Fraser, et al., Astrophys. J. 767, 1 (2013).
P. A. Pinto and R. G. Eastman, Astrophys. J. 530, 757 (2000).
M. Potashov, S. Blinnikov, P. Baklanov, and A. Dolgov, Mon. Not. R. Astron. Soc. Lett. 431, L98 (2013).
M. Sh. Potashov and A. V. Yudin, KIAM Preprint No. 82 (Keldysh Inst. Appl. Math., Moscow, 2022).
M. Sh. Potashov, S. I. Blinnikov, and E. I. Sorokina, Astron. Lett. 47, 204 (2021a).
M. Sh. Potashov et al., KIAM Preprint No. 87 (Keldysh Inst. Appl. Math., Moscow, 2021b).
J. L. Prieto, J. Brimacombe, A. J. Drake, and S. Howerton, Astrophys. J. Lett. 763, L27 (2013).
Yu. Ralchenko et al., NIST Atomic Spectra Database 2006. http://physics.nist.gov/asd3.
M. N. Saha, Proc. R. Soc. London 99, 135 (1921).
M. A. Skinner, J. C. Dolence, A. Burrows, D. Radice, and D. Vartanyan, Astrophys. J. Suppl. Ser. 241, 7 (2019).
V. V. Sobolev, Moving Envelopes of Stars (Harvard Univ., Cambridge, 1960; Leningr. Gos. Univ., Leningrad, 1947).
E. I. Sorokina and S. I. Blinnikov, arXiv astro-ph/0212187 (2002).
E. Urvachev and S. Glazyrin, Math. Model. Comput. Simul. 14, 633 (2022).
E. Urvachev, D. Shidlovski, N. Tominaga, S. Glazyrin, and S. Blinnikov, Astrophys. J. Suppl. Ser. 256, 8 (2021).
E. M. Urvachev, S. I. Blinnikov, S. I. Glazyrin, and P. V. Baklanov, Astron. Lett. 48, 20 (2022).
N. M. H. Vaytet, E. Audit, B. Dubroca, and F. Delahaye, J. Quant. Spectrosc. Radiat. Transfer 112, 1323 (2011).
D. A. Verner et al., arXiv astro-ph/9601009 (1996).
A. Vlasis, L. Dessart, and E. Audit, Mon. Not. R. Astron. Soc. 458, 1253 (2016).
Ya. B. Zel’dovich and Yu. P. Raizer, Physics of Shock Waves and High-Temperature Hydrodynamic Phenomena (Nauka, Moscow, 1966; Academic, New York, 1966, 1967).
ACKNOWLEDGMENTS
We thank the anonymous referees for their valuable remarks that allowed the SN 2009ip model and the content of the paper to be improved.
Funding
The work of E. M. Urvachev, S. I. Glazyrin, and D. S. Shidlovski on the development of the FRONT code and the simulations of SN 2009ip was supported by RSF grant no. 19-12-00229. The work of S. I. Blinnikov on the analysis of the light curves was supported by RSF grant no. 21-11-00362.
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Urvachev, E.M., Blinnikov, S.I., Glazyrin, S.I. et al. Comparative Modeling of the 2012b Outburst of Supernova 2009ip. Astron. Lett. 49, 454–464 (2023). https://doi.org/10.1134/S1063773723080054
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DOI: https://doi.org/10.1134/S1063773723080054