Zobrazeno 1 - 7
of 7
pro vyhledávání: '"Gao‐Chao Liu"'
Autor:
Peng Zong, Jian-Ning Fu, Jie Su, Xueying Hu, Bo Zhang, Jiaxin Wang, Gao-Chao Liu, Gang Meng, Gianni Catanzaro, Antonio Frasca, Haotian Wang, Weikai Zong
Publikováno v:
The Astronomical Journal, Vol 167, Iss 5, p 227 (2024)
We conduct an asteroseismological analysis on the non-Blazhko ab-type RR Lyrae star EPIC 248846335, employing the Radial Stellar Pulsations module of the Modules for Experiments in Stellar Astrophysics based on the set of stellar parameters. The atmo
Externí odkaz:
https://doaj.org/article/7f765bb757dd4216b971342286b9bf89
Publikováno v:
The Astrophysical Journal, Vol 944, Iss 1, p 88 (2023)
We present a sample of 135,873 RR Lyrae stars (RRLs) with precise photometric metallicity and distance estimates from our newly calibrated P – ϕ _31 – R _21 –[Fe/H]/ P – R _21 –[Fe/H] and G -band absolute magnitude–metallicity relations.
Externí odkaz:
https://doaj.org/article/7fb8e09650ec4419a27c0118be7e32d0
Autor:
Jia-Lu Nie, Hai-Jun Tian, Xi-Dong Wang, Morgan Fouesneau, Hans-Walter Rix, Ted von Hippel, Dan Qiu, Gao-Chao Liu
We analyze 4\,050 wide binary star systems involving a white dwarf (WD) and usually a main sequence (MS) star, drawn from the large sample assembled by \citet[][hereafter, T20]{Tian_2020}. Using the modeling code BASE-9, we determine the system's age
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9560668ebb244776ee45eec93b94af1d
In a semi-numerical model of reionization, the evolution of ionization fraction is simulated approximately by the ionizing photon to baryon ratio criterion. In this paper we incorporate a semi-analytical model of galaxy formation based on the Millenn
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::db14d0855b66d27f504a3c98d7030f99
Publikováno v:
Research in Astronomy & Astrophysics; Apr2013, Vol. 13 Issue 4, p373-386, 14p
Publikováno v:
physica status solidi (b). 153:K167-K170
On deduit une formule pour les parametres de resonance paramagnetique electronique g II et g⊥, et D. Pour MgO: Cr 3+ , les resultats theoriques sont en bon accord avec les experiences
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b07e95472ccd2ac34f5e8af1ba8f9c78
https://doi.org/10.1002/pssb.2221530252
https://doi.org/10.1002/pssb.2221530252
Publikováno v:
Journal of Physics: Condensed Matter; 11/21/1994, Vol. 6 Issue 47, p1-1, 1p