Zobrazeno 1 - 10
of 375
pro vyhledávání: '"Helium flash"'
Akademický článek
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We assume that the strong convection during core helium flash of low mass red giant branch (RBG) stars excite waves that propagate to the envelope, and find that the energy that these waves deposit in the envelope causes envelope expansion and bright
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::783415fe8fe7ed7ca4932733702e85c7
http://arxiv.org/abs/2106.00582
http://arxiv.org/abs/2106.00582
We report novel observational evidence on the evolutionary status of lithium-rich giant stars by combining asteroseismic and lithium abundance data. Comparing observations and models of the asteroseismic gravity-mode period spacing $����_{1}$
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2512ff223b7992f6ac6f6ae1d3912255
http://arxiv.org/abs/2104.12070
http://arxiv.org/abs/2104.12070
Autor:
A. E. Lynas-Gray
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 8 (2021)
There are a number of reasons for studying hot subdwarf pulsation; the most obvious being that these stars remain a poorly understood late-stage of stellar evolution and knowledge of their interior structure, which pulsation studies reveal, constrain
Autor:
Yu. A. Fadeyev
Stellar evolution calculations for population II stars with initial composition $Y_0=0.25$, $Z_0=10^{-3}$ and the initial stellar mass $M_0 = 0.82M_\odot$ were carried out from the main sequence to the white dwarf stage. Twelve AGB and post--AGB evol
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bfc1407fae00ec19a02f7d4b3a1f84aa
Akademický článek
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Autor:
C. K. Li, Jianrong Shi, Jinghua Zhang, Xianfei Zhang, Hong-Liang Yan, Yaguang Li, Yan Li, Shaolan Bi, Shuai Liu, Qi Gao, Gang Zhao
Publikováno v:
Zhang, J, Shi, J R, Yan, H L, Li, Y, Gao, Q, Li, C Q, Zhang, X, Liu, S, Bi, S, Zhao, G & Li, Y 2021, ' Lithium Evolution of Giant Stars Observed by LAMOST and Kepler ', Astrophysical Journal Letters, vol. 919, no. 1, L3 . https://doi.org/10.3847/2041-8213/ac224c
Mapping lithium evolution for evolved stars will provide restrictions and constraints on the fundamental stellar interior physical processes, which further shed light on our understanding of the theory of stellar structure and evolution. Based on a s
Publikováno v:
Arias Montano. Repositorio Institucional de la Universidad de Huelva
instname
instname
A radial velocity follow-up of the long-period sdOB+G1V type spectroscopic binary SB 744 revealed strong lines of fluorine and lead in the optical spectrum of the sdOB star and subsolar metallicity in the G1V companion. With high-quality observations
Publikováno v:
The Astrophysical Journal Letters. 915:L34
We propose a common envelope evolution (CEE) scenario where a red giant branch (RGB) star engulfs a planet during its core helium flash to explain the puzzling system WD 1856+534 where a planet orbits a white dwarf (WD) of mass 0.52Mo with an orbital