Zobrazeno 1 - 10
of 37
pro vyhledávání: '"V. P. Utrobin"'
Autor:
N. N. Chugai, V. P. Utrobin
Publikováno v:
Astronomy Letters. 48:275-283
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::202c148e239216f6069f03f7d1011feb
https://doi.org/10.1134/s1063773722060020
https://doi.org/10.1134/s1063773722060020
Autor:
T Kangas, C Fransson, J Larsson, K France, R A Chevalier, R P Kirshner, P Lundqvist, S Mattila, J Sollerman, V P Utrobin
We present spectroscopy of the ejecta of SN 1987A in 2017 and 2018 from the Hubble Space Telescope and the Very Large Telescope, covering the wavelength range between $1150$ and $10000$ {\AA}. At 31 years, this is the first epoch with coverage over t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::68697f2636b0344cacf4dabeb5920139
http://arxiv.org/abs/2112.11158
http://arxiv.org/abs/2112.11158
Autor:
V. P. Utrobin, Nikolai Chugai
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 490:2042-2049
The enigmatic type IIP SN 2016X demonstrates the unprecedented asphericity in the nebular H-alpha line profile, the absence of nebular [O I] emission, and the unusual occultation effect due to the internal dust. The hydrodynamic modelling of the bolo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::57087150cabd0c09d0cd7bf91db92abe
https://doi.org/10.1093/mnras/stz2716
https://doi.org/10.1093/mnras/stz2716
Autor:
Alexander Heger, T. Ertl, H.-Th. Janka, A. Menon, Annop Wongwathanarat, V. P. Utrobin, Ewald Müller
Six binary-merger progenitors of Supernova 1987A (SN 1987A) with properties close to those of the blue supergiant Sanduleak -69 202 are exploded by neutrino heating and evolved until long after shock breakout in three dimensions (3D), and continued f
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b3b59507b5c3ce5918c55d712b01e0a6
http://arxiv.org/abs/2102.09686
http://arxiv.org/abs/2102.09686
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 482:438-452
Based on the work of Menon & Heger (2017), we present the bolometric light curvesand spectra of the explosions of blue supergiant progenitors from binary mergers. We study SN 1987A and two other peculiar Type IIP supernovae: SN 1998A and SN 2006V. Th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::452e6069b3271f48938eca3cd7e8cc42
https://doi.org/10.1093/mnras/sty2647
https://doi.org/10.1093/mnras/sty2647
Autor:
Nikolai Chugai, V. P. Utrobin
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 472:5004-5010
We explore the well-observed type IIP SN 2013ej with peculiar luminosity evolution. It is found that the hydrodynamic model cannot reproduce in detail the bolometric luminosity at both the plateau and the radioactive tail. Yet the ejecta mass of 23-2
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::54a40f8736d77d22b28a545b496caea7
https://doi.org/10.1093/mnras/stx2415
https://doi.org/10.1093/mnras/stx2415
Autor:
P. V. Baklanov, V. P. Utrobin, I. V. Panov, A. V. Yudin, K V Manukovskiy, Sergei Blinnikov, D K Nadyozhin
Publikováno v:
Physics-Uspekhi. 59:796-806
Astrophysical research at the Institute for Theoretical and Experimental Physics (ITEP) is examined historically over a period of more than 30 years. The primary focus is on the supernova problem, starting with how it was approached in the classical
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::afbef3d847167ab81861e638cea561f8
https://doi.org/10.3367/ufne.2016.04.037810
https://doi.org/10.3367/ufne.2016.04.037810
With the same method as used previously, we investigate neutrino-driven explosions of a larger sample of blue supergiant models. The larger sample includes three new presupernova stars. The results are compared with light-curve observations of the pe
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f2e2196ad398973eba627ea003ca51cb
The importance of allowance for the time-dependent effect in the kinetics at the photospheric phase during a supernova explosion has been confirmed by several independent research groups. The time-dependent effect provides a higher degree of hydrogen
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ee2617e37689e882ca47966a922b1499
http://arxiv.org/abs/1707.02177
http://arxiv.org/abs/1707.02177
Autor:
V. V. Lukin, N. I. Shakura, V. P. Utrobin, Konstantin Postnov, Konstantin Malanchev, V. M. Chechetkin
We present the results of 3D-hydrodynamical simulations of accretion flow in the eclipsing dwarf nova V1239 Her in quiescence. The model includes the optical star filling its Roche lobe, a gas stream emanating from the inner Lagrangian point of the b
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::89117774cdc73f49622b975d4ef45814
http://arxiv.org/abs/1702.00587
http://arxiv.org/abs/1702.00587