Zobrazeno 1 - 8
of 8
pro vyhledávání: '"Baklanov, Petr V."'
Autor:
Singh, Avinash, Sahu, D. K., Anupama, G. C., Kumar, Brajesh, Kumar, Harsh, Yamanaka, Masayuki, Baklanov, Petr V., Tominaga, Nozomu, Blinnikov, Sergei I., Maeda, Keiichi, Dutta, Anirban, Bhalerao, Varun, Anche, Ramya M., Barway, Sudhanshu, Akitaya, Hiroshi, Nakaoka, Tatsuya, Kawabata, Miho, Kawabata, Koji S, Sasada, Mahito, Takagi, Kengo, Maehara, Hiroyuki, Isogai, Keisuke, Kino, Masaru, Taguchi, Kenta, Nagao, Takashi
High cadence ultraviolet, optical and near-infrared photometric and low-resolution spectroscopic observations of the peculiar Type II supernova (SN) 2018hna are presented. The early phase multiband light curves exhibit the adiabatic cooling envelope
Externí odkaz:
http://arxiv.org/abs/1908.07807
Autor:
Tanaka, Masaomi, Tominaga, Nozomu, Morokuma, Tomoki, Yasuda, Naoki, Furusawa, Hisanori, Baklanov, Petr V., Blinnikov, Sergei I., Moriya, Takashi J., Doi, Mamoru, Jiang, Ji-an, Kato, Takahiro, Kikuchi, Yuki, Kuncarayakti, Hanindyo, Nagao, Tohru, Nomoto, Ken'ichi, Taniguchi, Yuki
We present rapidly rising transients discovered by a high-cadence transient survey with Subaru telescope and Hyper Suprime-Cam. We discovered five transients at z=0.384-0.821 showing the rising rate faster than 1 mag per 1 day in the restframe near-u
Externí odkaz:
http://arxiv.org/abs/1601.03261
Autor:
Moriya, Takashi J., Blinnikov, Sergei I., Baklanov, Petr V., Sorokina, Elena I., Dolgov, Alexander D.
Publikováno v:
Monthly Notices of the Royal Astronomical Society, Volume 430, Issue 2, p.1402-1407 (2013)
We numerically investigate light curves (LCs) of shocked circumstellar shells which are suggested to reproduce the observed LC of superluminous SN 2006gy analytically. In the previous analytical model, the effects of the recombination and the bolomet
Externí odkaz:
http://arxiv.org/abs/1301.0355
Autor:
Moriya, Takashi, Tominaga, Nozomu, Blinnikov, Sergei I., Baklanov, Petr V., Sorokina, Elena I.
Publikováno v:
Monthly Notices of the Royal Astronomical Society, Volume 415, Issue 1, pp. 199-213 (2011)
We calculate multicolor light curves (LCs) of supernovae (SNe) from red supergiants (RSGs) exploded within dense circumstellar medium (CSM). Multicolor LCs are calculated by using a multi-group radiation hydrodynamics code STELLA. If CSM is dense eno
Externí odkaz:
http://arxiv.org/abs/1009.5799
Akademický článek
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Autor:
Moriya, Takashi J., Tominaga, Nozomu, Blinnikov, Sergei I., Baklanov, Petr V., Sorokina, Elena I.
Publikováno v:
Proceedings of the International Astronomical Union; Apr2011 Supplement, Vol. 7 Issue S279, p54-57, 4p
Akademický článek
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Autor:
Moriya, Takashi, Tominaga, Nozomu, Blinnikov, Sergei I., Baklanov, Petr V., Sorokina, Elena I.
Publikováno v:
Monthly Notices of the Royal Astronomical Society; Aug2012, Vol. 424 Issue 3, p2400-2400, 1p