Zobrazeno 1 - 10
of 73
pro vyhledávání: '"Hai-Liang Chen"'
Telomere-to-telomere genome assembly of a male goat reveals variants associated with cashmere traits
Autor:
Hui Wu, Ling-Yun Luo, Ya-Hui Zhang, Chong-Yan Zhang, Jia-Hui Huang, Dong-Xin Mo, Li-Ming Zhao, Zhi-Xin Wang, Yi-Chuan Wang, EEr He-Hua, Wen-Lin Bai, Di Han, Xing-Tang Dou, Yan-Ling Ren, Renqing Dingkao, Hai-Liang Chen, Yong Ye, Hai-Dong Du, Zhan-Qiang Zhao, Xi-Jun Wang, Shan-Gang Jia, Zhi-Hong Liu, Meng-Hua Li
Publikováno v:
Nature Communications, Vol 15, Iss 1, Pp 1-20 (2024)
Abstract A complete goat (Capra hircus) reference genome enhances analyses of genetic variation, thus providing insights into domestication and selection in goats and related species. Here, we assemble a telomere-to-telomere (T2T) gap-free genome (2.
Externí odkaz:
https://doaj.org/article/78ee5eea4c8c4b08a52e6972705d4cee
Publikováno v:
The Astrophysical Journal, Vol 951, Iss 2, p 91 (2023)
The formation path to ultracompact X-ray binaries (UCXBs) with black hole (BH) accretors is still unclear. In the classical formation scenario, it is difficult to eject the massive envelope of the progenitor star of the BH via the common envelope pro
Externí odkaz:
https://doaj.org/article/4cd8a5460cb948f0a00e1b9a29f24726
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 505:3514-3519
Most subdwarf B (sdB) + Helium white dwarf (He WD) binaries are believed to be formed from a particular channel. In this channel, the He WDs are produced first from red giants (RGs) with degenerate cores via stable mass transfer and sdB stars are pro
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 502:383-389
Binaries that evolved from red giant (RG) binaries through stable Roche lobe overflow follow the mass–orbital period relation if the donor’s core is degenerate. This relation is important for the studies of long orbital period blue stragglers, su
Publikováno v:
Chen, H L, Tauris, T M, Chen, X & Han, Z 2022, ' Investigating the Stability of Mass Transfer in Neutron Star–helium White Dwarf Binaries ', Astrophysical Journal, vol. 930, no. 2, 134 . https://doi.org/10.3847/1538-4357/ac6608
Neutron star–helium white dwarf (NS+He WD) binaries are important evolutionary products of close-orbit binary star systems. They are often observed as millisecond pulsars and may continue evolving into ultracompact X-ray binaries (UCXBs) and contin
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::09cfa3ba9e27cfc9e7ec3b6cfb1933c7
https://vbn.aau.dk/da/publications/3db68eea-07bf-470e-b507-d9cb7e657e26
https://vbn.aau.dk/da/publications/3db68eea-07bf-470e-b507-d9cb7e657e26
Publikováno v:
The Journal of Physical Chemistry C. 123:28008-28014
Iron hydrides can be formed under high pressure and have special physical and chemical properties. Structures and stabilities of FeXSeHY (X = 1–2, Y = 1–6) hydrides under high pressure were studied using a genetic algorithm method combined with D
Autor:
Ping Li, Qianhui Zeng, Huan Tong Wan, Rui Chun Zhou, Shiang-Lin Huang, Yuelin Li, Derun Lin, Hai Liang Chen, Miao Bao, Wenhua Liu, Xianyan Wang, Xi Chen, You Sheng Xiao, Fuxin Wu
Publikováno v:
Ocean & Coastal Management. 169:147-156
Bridging information gaps in an animal's habitat configuration is an explicit challenge in planning habitat protection actions (HPAs) for marine megafauna species near sites of intense anthropogenic activity. This challenge is further complicated by
Publikováno v:
Physics Letters A. 383:774-780
Stable structures of uranium hydrides at 0–550 GPa were studied using genetic algorithm (GA) combined with density functional theory calculations. We investigated two stoichiometries of U–H system, UH4 and UH10 at high pressure, and properties of
Publikováno v:
The Astrophysical Journal. 935:9
The evolution and the stability of mass transfer of CO+He white dwarf (WD) binaries are not well understood. Observationally they may emerge as AM CVn binaries and are important gravitational wave (GW) emitters. In this work, we have modeled the evol
Publikováno v:
The Astrophysical Journal. 933:118