Zobrazeno 1 - 10
of 412
pro vyhledávání: '"Tarasova, T."'
Autor:
Khmyrov, R. S., Podrabinnik, P. A., Tarasova, T. V., Gridnev, M. A., Korotkov, A. D., Grigoriev, S. N., Kurmysheva, A. Yu., Kovalev, O. B., Gusarov, A. V.
Metals in amorphous state are promising for the use as structural materials due to their superior properties related to the absence of grain boundaries and dislocations.Obtaining the amorphous state requires quenching with a high cooling rate.In conv
Externí odkaz:
http://arxiv.org/abs/2211.17140
Autor:
Slunyaev, A. V., Tarasova, T. V.
Synchronous collisions between a large number of solitons are considered in the context of a statistical description. It is shown that during the interaction of solitons of the same signs the wave field is effectively smoothed out. When the number of
Externí odkaz:
http://arxiv.org/abs/2208.06220
Autor:
Skopal, A., Shugarov, S. Yu., Munari, U., Masetti, N., Marchesini, E., Komzik, R. M., Kundra, E., Shagatova, N., Tarasova, T. N., Buil, C., Boussin, C., Shenavrin, V. I., Hambsch, F. -J., Dallaporta, S., Frigo, A., Garde, O., Zubareva, A., Dubovský, P. A., Kroll, P.
Publikováno v:
A&A 636, A77 (2020)
The star V426 Sge (HBHA~1704-05), originally classified as an emission-line object and a semi-regular variable, brightened at the beginning of August 2018, showing signatures of a symbiotic star outburst. We aim to confirm the nature of V426 Sge as a
Externí odkaz:
http://arxiv.org/abs/2003.10135
Autor:
Tatarnikova, A. A., Burlak, M. A., Kolotilov, E. A., Metlova, N. V., Shenavrin, V. I., Shugarov, S. Yu., Tarasova, T. N., Tatarnikov, A. M.
A new set of low-resolution spectral and UBVJHKL-photometric observations of the symbiotic nova PU Vul is presented. The binary has been still evolving after the symbiotic nova outburst in 1977 and now it's in the nebular stage. It is found that the
Externí odkaz:
http://arxiv.org/abs/1803.05739
Autor:
Skopal, A., Shugarov, S. Yu., Sekeráš, M., Wolf, M., Tarasova, T. N., Teyssier, F., Fujii, M., Guarro, J., Garde, O., Graham, K., Lester, T., Bouttard, V., Lemoult, T., Sollecchia, U., Montier, J., Boyd, D.
Publikováno v:
A&A 604, A48 (2017)
AG Peg is known as the slowest symbiotic nova, which experienced its nova-like outburst around 1850. After 165 years, during June of 2015, it erupted again showing characteristics of the Z And-type outburst. The primary objective is to determine basi
Externí odkaz:
http://arxiv.org/abs/1705.00076
Publikováno v:
In Composites Part A February 2022 153
Akademický článek
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Autor:
Tarasova, T. N.
Spectroscopic observations of the hybrid V458 Vul obtained between days 9 and 778 after the brightness maximum are analyzed. Short-period, daily profile variations of forbidden [FeVII] iron lines were detected in the nebular phase, as well as a long-
Externí odkaz:
http://arxiv.org/abs/1508.03990
Publikováno v:
In International Journal of Fatigue November 2020 140
Akademický článek
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