Zobrazeno 1 - 10
of 58
pro vyhledávání: '"Li-Yong Zhou"'
Publikováno v:
In Chinese Astronomy and Astrophysics January-March 2024 48(1):142-160
Autor:
QIN Song, LI Shuang-hu, ZHOU Jian-qiao, YANG Jia-lin, WEI Xiang, LI Yong, ZHOU Ao, XIA Guang-ming
Publikováno v:
Cailiao Baohu, Vol 56, Iss 2, Pp 70-76 (2023)
In order to design and prepare hard coating for the flue gas turbine transition ring,and to ensure the long-term stable operation of the flue gas turbine,three kinds of Cr3C2-NiCr hard coatings were designed and prepared on the surface of 304L al
Externí odkaz:
https://doaj.org/article/3a42db72abfa4f9d911c7a5a0c1756fe
Autor:
Yi-sui Sun, Li-yong Zhou
This book provides a brief introduction to some basic but important problems in celestial mechanics, and particularly in the few-body problem, such as the permissible and forbidden region of motion, the evolution of moment of inertia of a system, and
The Yarkovsky effect plays an important role in the motions of small celestial bodies. Increasingly improving observations bring the need of high-accuracy modelling of the effect. Using a multiphysics software COMSOL, we model the diurnal Yarkovsky e
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::71545efafaa1ae0758ac70c9c0b8895f
http://arxiv.org/abs/2206.10921
http://arxiv.org/abs/2206.10921
The long-standing co-orbital asteroids have been thought to be the possible source of zodiacal dust ring around the orbit of Venus, but inconsistent conclusions on the orbital stability thus existence of Venus Trojans are found in literature. We pres
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::31381cec308dc142ffded2f11ecd98f1
http://arxiv.org/abs/2206.06114
http://arxiv.org/abs/2206.06114
Publikováno v:
Astronomy & Astrophysics. 673:A5
The mass-independent isotopic signatures of planetary bodies have been widely used to trace the mixing process that occurred during planet formation. The observed isotopic variations among meteorite parent bodies have been further linked to the model
Akademický článek
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Publikováno v:
Monthly Notices of the Royal Astronomical Society. 493:1447-1460
Based on a linearized model of the Yarkovsky effect, we investigate in this paper the dependence of the semimajor axis drift $\Delta a$ of a celestial body on its size, spinning obliquity, initial orbit and thermal parameters on its surface. With app
Considering the huge computational resources required by smoothed particle hydrodynamics (SPH) simulations and the overestimation of post-collision materials from perfect merging, we develop a statistical method to deal with collisions during the for
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::274c98eb1bbd93f406a9d32d8ed881f7
http://arxiv.org/abs/2105.10105
http://arxiv.org/abs/2105.10105
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 488:5604-5614
The presented work investigates the possible formation of terrestrial planets in the habitable zone (HZ) of the exoplanetary system HD 141399. In this system, the HZ is located approximately between the planets c (a = 0.7 au) and d (a = 2.1 au). Exte