Zobrazeno 1 - 9
of 9
pro vyhledávání: '"Dmitry Shishkin"'
Publikováno v:
The Astrophysical Journal, Vol 975, Iss 2, p 281 (2024)
Analyzing images of the Cygnus Loop, a core-collapse supernova (CCSN) remnant, in different emission bands, we identify a point-symmetrical morphology composed of three symmetry axes that we attribute to shaping by three pairs of jets. The main jet a
Externí odkaz:
https://doaj.org/article/17a2afff4cc94920933667bc74ed683a
Publikováno v:
The Astrophysical Journal, Vol 969, Iss 2, p 163 (2024)
We conduct one-dimensional stellar-evolution simulations of stars with zero-age main-sequence (ZAMS) masses of M _ZAMS = 8.8 − 9.45 M _⊙ toward core collapse by electron capture and find that the convective zone of the precollapse core can supply
Externí odkaz:
https://doaj.org/article/abb5e80c4d0b412a89012fa581647fbb
Autor:
Dmitry Shishkin, Noam Soker
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 522:438-445
We examine the binding energies of massive stripped-envelope core collapse supernova (SECCSN) progenitors with the stellar evolution code MESA, and find that the jittering jets explosion mechanism is preferred for explosions where carbon-oxygen cores
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4f9f1f9fcacf1a83e26ef6a7949d37c7
https://doi.org/10.1093/mnras/stad889
https://doi.org/10.1093/mnras/stad889
Autor:
Igor Burlakov, Dmitry Shishkin, Svetlana Vydumkina, Denis Kapitanenko, Yuliy Kalpin, Pavel Petrov
Publikováno v:
Procedia Manufacturing. 50:520-528
The paper describes the existing methods for constructing hardening curves based on the torsion of continuous cylindrical and tubular samples. The advantages and disadvantages of the known methods are observed. It resulted in the development of an ap
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::fb5599c18cd11bdcd96f406c58b8ab54
https://doi.org/10.1016/j.promfg.2020.08.094
https://doi.org/10.1016/j.promfg.2020.08.094
Autor:
Dmitry Shishkin, Noam Soker
We conduct one dimensional (1D) stellar evolution simulations of non-rotating stars with initial masses in the range of $11-48 M_\odot$ to the time of core collapse and, using a criterion on the specific angular momentum fluctuations in the inner con
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5ac195685bc14a446857ffaff81185e5
http://arxiv.org/abs/2112.10697
http://arxiv.org/abs/2112.10697
Autor:
Dmitry Shishkin, Noam Soker
We conduct one-dimensional stellar evolution simulations in the mass range $13-20 M_{\odot}$ to late core collapse times and find that an inner vigorous convective zone with large specific angular momentum fluctuations appears at the edge of the iron
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5e7253cf4b9f334078b26e8d1fb46a33
Autor:
Galina Pankova, Dmitry Shishkin
Publikováno v:
Век информации (сетевое издание). 4
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1d3c938c636ae6416665bf25252930c6
https://doi.org/10.33941/age-info.com41(10)1
https://doi.org/10.33941/age-info.com41(10)1
Autor:
Dmitry Shishkin
Publikováno v:
Public Finance Review. 41:473-488
A closer look at the estimating procedures that have been used to examine the empirical evidence of weak fiscal incentives at the local level in Russia in 1990s shows serious flaws in the treatment of proceeds from shared revenue sources with differe
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::fc0b0c86ebebe217d0cd8fbc5976a12e
https://doi.org/10.1177/1091142113475698
https://doi.org/10.1177/1091142113475698
Publikováno v:
International Journal of Economics and Business Research. 3:609
During the job application and interview process, there is a natural tendency for applicants to stress attributes that they possess and that they also believe are being sought by hiring organisations. Due to cultural differences, applicants may be un
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::451a5ef31fb5da877b625a31165a54e3
https://doi.org/10.1504/ijebr.2011.043056
https://doi.org/10.1504/ijebr.2011.043056