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pro vyhledávání: '"Yaotian Zeng"'
Single-degenerate (SD) binary systems composed of a white dwarf and a non-degenerate helium (He)-star companion have been proposed as the potential progenitors of Type Ia supernovae (SNe Ia). The He-star companions are expected to survive the SN Ia e
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bae7875fc1de4070e13a75c70e882005
http://arxiv.org/abs/2202.07676
http://arxiv.org/abs/2202.07676
The sub-Chandrasekhar mass double-detonation (DDet) scenario is a contemporary model for SNe Ia. The donor star in the DDet scenario is expected to survive the explosion and to be ejected at the high orbital velocity of a compact binary system. For t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9968a0d81b687d50c58d160abe4fde7a
http://arxiv.org/abs/2109.09980
http://arxiv.org/abs/2109.09980
Autor:
Zheng-Wei Liu, Yaotian Zeng
The nature of the progenitors and explosion mechanism of Type Iax supernovae (SNe Iax) remain a mystery. The single-degenerate (SD) systems that involve the incomplete pure deflagration explosions of near-Chandrasekhar-mass white dwarfs (WDs) have re
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9f51de9b38d99655026586dcc596b84b
http://arxiv.org/abs/2011.07691
http://arxiv.org/abs/2011.07691
Autor:
Curtis McCully, Saurabh W. Jha, Richard A. Scalzo, D. Andrew Howell, Ryan J. Foley, Yaotian Zeng, Zheng-Wei Liu, Griffin Hosseinzadeh, Lars Bildsten, Adam G. Riess, Robert P. Kirshner, G. H. Marion, Yssavo Camacho-Neves
Publikováno v:
The Astrophysical Journal. 925:138
Type Iax supernovae represent the largest class of peculiar white-dwarf supernovae. The type Iax SN~2012Z in NGC 1309 is the only white dwarf supernova with a detected progenitor system in pre-explosion observations. Deep \textit{Hubble Space Telesco
Publikováno v:
The Astrophysical Journal. 898:12
Type Iax supenovae (SNe Iax) are an important sub-luminous class of SNe Ia. However, their progenitors and explosion mechanism have not been understood yet. It has been suggested that SNe Iax may be produced from weak deflagration explosions of Chand