Zobrazeno 1 - 10
of 110
pro vyhledávání: '"E I, Sorokina"'
Publikováno v:
Astronomy Letters. 47:204-213
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 supernova ejecta it also depends on the expansion velocity gradient, because the Doppler eff
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d60c6bce28e075c50bc3d5bdafec87b7
https://doi.org/10.1134/s1063773721030051
https://doi.org/10.1134/s1063773721030051
Autor:
Melina C. Bersten, Alexey Tolstov, Ken'ichi Nomoto, E. I. Sorokina, Sergei Blinnikov, T. Suzuki
Publikováno v:
Proceedings of the International Astronomical Union. 12:39-43
The physical origin of Type-I (hydrogen-less) superluminous supernovae (SLSNe-I), whose luminosities are 10 to 500 times higher than normal core-collapse supernovae, remains still unknown. Thanks to their brightness, SLSNe-I would be useful probes of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c22701bb41e17905a9afe87a14be8efb
https://doi.org/10.1017/s174392131700343x
https://doi.org/10.1017/s174392131700343x
Publikováno v:
Space Science Reviews. 214
Superluminous supernovae are a new class of supernovae that were recognized about a decade ago. Both observational and theoretical progress has been significant in the last decade. In this review, we first briefly summarize the observational properti
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bc04f9304d0ae5ccd0475173cb040bf7
https://doi.org/10.1007/s11214-018-0493-6
https://doi.org/10.1007/s11214-018-0493-6
Autor:
Markus Kromer, Wolfgang Hillebrandt, E. I. Sorokina, S. Taubenberger, U. M. Noebauer, P. V. Baklanov, Sergei Blinnikov
Upcoming high-cadence transient survey programmes will produce a wealth of observational data for Type Ia supernovae. These data sets will contain numerous events detected very early in their evolution, shortly after explosion. Here, we present synth
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cefe6a2c0185a7188f45e986ab176ab1
http://arxiv.org/abs/1706.03613
http://arxiv.org/abs/1706.03613
Publikováno v:
Russian Journal of Inorganic Chemistry. 58:861-865
Phase equilibria in the LiF-KCl-KVO3-K2MoO4-LiKMoO4 stable pentatope of the Li,K‖F,Cl,VO3,MoO4 reciprocal five-component system were studied using differential thermal analysis (DTA). A eutectic was found to have a composition (mol %) of 50.0 LiF,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b19972ccd585e1f310fe050da8fc1066
https://doi.org/10.1134/s0036023613020265
https://doi.org/10.1134/s0036023613020265
Publikováno v:
HIGH ENERGY DENSITY PHYSICS
The first powerful burst of photon radiation in a supernova appears when the shock front is a few photon mean-free paths below the star photosphere. This is called “shock breakout” and it is the first observable event after the neutrino and gravi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::246c15aa567ce107d4aa8fefffba67b6
https://doi.org/10.1016/j.hedp.2012.09.004
https://doi.org/10.1016/j.hedp.2012.09.004
Publikováno v:
Russian Journal of Inorganic Chemistry. 58:96-101
The Li,K‖Cl,VO3,MoO4 system was partitioned into simplexes using graph theory, and the tree of phases for this system was constructed. The equations of the main reactions describing the chemical interaction in the quaternary mutual systems Li,K‖F
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::bdd930fd1cd7ab1a21a05b668c573cac
https://doi.org/10.1134/s0036023613010208
https://doi.org/10.1134/s0036023613010208
We investigate the consequences of fairly normal Type Ia supernovae being embedded in compact and dense envelopes of carbon and oxygen rich circumstellar material by means of detailed radiation hydrodynamic simulations. Our main focus rests on explor
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ef3ca5c41ec5d32827ed31bac3fa39a3
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 415:199-213
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:
https://explore.openaire.eu/search/publication?articleId=doi_________::eab655010fa4354d32c8f9259180f706
https://doi.org/10.1111/j.1365-2966.2011.18689.x
https://doi.org/10.1111/j.1365-2966.2011.18689.x
Publikováno v:
Proceedings of the International Astronomical Union. 7:54-57
Red supergiants (RSGs) are progenitors of Type IIP supernovae (SNe). It is suggested that RSGs can experience a mass loss with a very high mass-loss rate (even as high as 0.01 M⊙ yr−1) due to, e.g., dynamical instabilities of their envelopes (e.g
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::bb70f5af550a339bb157a1988c495534
https://doi.org/10.1017/s1743921312012689
https://doi.org/10.1017/s1743921312012689