Search Results - "Sorokina, E. I."

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  1. 1

    Opacity of Ejecta in Calculations of Supernova Light Curves by Potashov, M. Sh, Blinnikov, S. I., Sorokina, E. I.

    Published in Astronomy letters (01-04-2021)
    “…The plasma opacity in stars depends mainly on the local state of matter (the density, temperature, and chemical composition at the point of interest), but in…”
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  2. 2

    Hydrogenless superluminous supernova PTF12dam in the model of an explosion inside an extended envelope by Baklanov, P. V., Sorokina, E. I., Blinnikov, S. I.

    Published in Astronomy letters (01-03-2015)
    “…Amodel of a supernova explosion inside a dense extended hydrogenless envelope is proposed to explain the properties of the light curve for one of the…”
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    LiF-KCl-KVO3-K2MoO4-LiKMoO4 stable pentatope by Sorokina, E. I., Gubanova, T. V., Garkushin, I. K.

    Published in Russian journal of inorganic chemistry (01-07-2013)
    “…Phase equilibria in the LiF-KCl-KVO 3 -K 2 MoO 4 -LiKMoO 4 stable pentatope of the Li,K‖F,Cl,VO 3 ,MoO 4 reciprocal five-component system were studied using…”
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  4. 4

    Opacity of Ejecta in Calculations of Supernova Light Curves by Potashov, M. Sh, Blinnikov, S. I, Sorokina, E. I

    Published 22-10-2024
    “…Astron. Lett., vol. 47, no. 4, pp. 204-213, Apr. 2021 The plasma opacity in stars depends mainly on the local state of matter (the density, temperature, and…”
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  5. 5

    X-ray emission of young SN Ia remnants as a probe for an explosion model by Kosenko, D.I, Sorokina, E.I, Blinnikov, S.I, Lundqvist, P

    Published in Advances in space research (2004)
    “…We present results of hydrodynamical simulations of young supernova remnants. To model the ejecta, we use several models (discussed in the literature) of type…”
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  6. 6

    Chemical interaction in the quaternary mutual systems Li,K‖F,Cl,MoO4 and Li,K‖F(Cl),VO3,MoO4 by Sorokina, E. I., Garkushin, I. K., Gubanova, T. V.

    “…The Li,K‖Cl,VO 3 ,MoO 4 system was partitioned into simplexes using graph theory, and the tree of phases for this system was constructed. The equations of the…”
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  7. 7

    Time-dependent thermal X-ray afterglows from GRBS by Kosenko, D.I., Blinnikov, S.I., Postnov, K.A., Lundqvist, P., Sorokina, E.I.

    Published in Advances in space research (2004)
    “…Time-dependent thermal X-ray spectra are calculated from physically plausible conditions around GRB. It is shown that account for time-dependent ionization…”
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  8. 8

    X-ray emission lines in the early afterglows of gamma-ray bursts by Kosenko, D I, Blinnikov, S I, Postnov, K A, Lundqvist, P, Sorokina, E I

    Published in Astronomy letters (01-04-2003)
    “…We computed the thermal time-dependent X-ray spectrum of a hot plasma in the vicinity of a gamma-ray burst (GRB). An allowance for time-dependent processes in…”
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  9. 9

    Burning regimes for thermonuclear supernovae and cosmological applications of SNe Ia by Sorokina, E I, Blinnikov, S I, Bartunov, O S

    Published in Astronomy letters (01-02-2000)
    “…The method of multigroup radiation hydrodynamics is used to compute light curves for thermonuclear supernovae. Opacities are computed by taking into account…”
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  10. 10

    The origin of the high-velocity circumstellar gas around SN 1998S by Chugai, N.N., Blinnikov, S.I., Fassia, A., Lundqvist, P., Meikle, W.P.S., Sorokina, E.I.

    “…Modelling of high-resolution Balmer line profiles in the early-time spectra of SN 1998S shows that the inferred fast (≈400 km s−1) circumstellar (CS) gas on…”
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  11. 11

    Dynamics and radiation of young type-Ia supernova remnants: Important physical processes by Sorokina, E I, Blinnikov, S I, Kosenko, D I, Lundqvist, P

    Published in Astronomy letters (01-11-2004)
    “…We analyze the physical processes that should be taken into account when modeling young type-Ia supernova remnants (SNRs) with ages of several hundred years in…”
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  12. 12

    Shock Breakout in Type II Plateau Supernovae: Prospects for High Redshift Supernova Surveys by Tominaga, N, Morokuma, T, Blinnikov, S. I, Baklanov, P, Sorokina, E. I, Nomoto, K

    Published 01-03-2011
    “…Shock breakout is the brightest radiative phenomenon in a supernova (SN) but is difficult to be observed owing to the short duration and X-ray/ultraviolet…”
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  13. 13

    Endothelin-1 as a risk factor causing cardiovascular pathology in young and middle-aged people employed under hazardous working conditions by I.A. Umnyagina, T.V. Blinova, L.A. Strakhova, V.V. Troshin, Yu.V. Ivanova, E.I. Sorokina

    Published in Analiz riska zdorovʹi͡u (01-06-2021)
    “…Our research goal was to reveal peculiarities related to changes in endothelin-1 contents in blood serum in young and middle-aged people exposed to…”
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    Time-dependent thermal effects in GRB afterglows by Postnov, K.A., Blinnikov, S.I., Kosenko, D.I., Sorokina, E.I.

    “…Time-dependent thermal effects should accompany standard non-thermal afterglows of GRB when γ-rays pass through inhomogeneous surroundings of the GRB site…”
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    The effect of contrast baths on the hemostatic function of patients with ischemic heart disease by Sorokina, E I, Ali, O

    “…Contrast baths effects on hemostasis were studied in 72 patients with postinfarction cardiosclerosis and stable angina pectoris. Hemostasis was assessed by…”
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  19. 19

    Supernova Explosions inside Carbon-Oxygen Circumstellar Shells by Blinnikov, S. I, Sorokina, E. I

    Published 22-09-2010
    “…Motivated by a recent discovery of Supernova 2010gx and numerical results of Fryer et al.(2010), we simulate light curves for several type I supernova models,…”
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