the National Natural Science Foundation of China(11973072/12233010).
The Free Core Nutation(FCN)is a rotational mode caused by non-alignment of the rotation axis of the core and of the mantle.Its period observed by VLBI and superconducting gravimetry is around 430 sidereal days(Sd)with...
the University of Kwa Zulu-Natal for financial support;University of Dar es Salaam;the Ministry of Education;Science and Technology-Tanzania(MOEST)for continuous support。
We establish new charged stellar models from the Einstein-Maxwell field equations for relativistic superdense objects outfitted with three layers.The core layer is described by a linear equation of state(EoS)describin...
financial support of the National Natural Science Foundation of China (No. 12073011);the National Key R&D Program of China (No. 2019YFA0706601)。
In this study, a new expansion of planetary disturbing function is developed for describing the resonant dynamics of minor bodies with arbitrary inclinations and semimajor axis ratios. In practice, the disturbing func...
supported by the Joint Research Fund in Astronomy(Grant Nos.U1631236,U2031203)under cooperative agreement between the National Natural Science Foundation of China(NSFC)and Chinese Academy of Sciences(CAS);NSFC(Grant No.11522325);the European Research Council(ERC)under the European Union’s Horizon 2020 research and innovation programme(CartographY GA.804752)。
The change of sound speed has been found at the base of the convection during the solar cycles,which can be used to constrain the solar internal magnetic field.We aim to check whether the magnetic field generated by t...
supported by the National Natural Science Foundation of China(Grant Nos.11673052 and 41661164034);the Pilot Project of the Chinese Academy of Sciences(No.XDB18010203)
Motivated by the desire to understand the rich dynamics of precessionally driven flow in a liquid planetary core, we investigate, through numerical simulations, the precessing fluid motion in a ro- taring cylindrical ...
supported by the Xinjiang Science Fund for Distinguished Young Scholars under Grant Nos. 2013721014 and 2014721015;the National Natural Science Foundation of China under Grant Nos. 11473024, 11363005 and 11163005
Using stellar evolutionary models, we investigate the effects of convective overshooting on naked helium stars. We find that a larger value of overshooting parameter δov results in a larger convective core, which pro...
supported by the Scientific and Technological Research Council of Turkey(TBTAK 112T989)
Grids of stellar evolution omy/astrophysics, such as planet hosting are required in many fields of astron- stars, binaries, clusters, chemically peculiar stars, etc. In this study, a grid of stellar evolution models w...
supported by the National Natural Science Foundation of China (Grant Nos. 10773029 and 10973015);the National Basic Research Program of China (973 program; Grant No. 2007CB815406);received funding from the exchange programme between Chinese Academy of Sciences and the Danish Rectors’ Conference (UniversitiesDenmark);Funding for the Stellar Astrophysics Centre is provided by The Danish National Research Foundation (Grant DNRF106);supported by the ASTERISK project (ASTERoseismic Investigations with SONG and Kepler) funded by the European Research Council (Grant No. 267864)
Local mixing-length theory is incapable of describing nonlocal phenom- ena in stellar convection, such as overshooting. Therefore standard solar models con- structed with local mixing-length theory significantly devia...
supported by the Belgian PRODEX program managed by the European Space Agency in collaboration with the Belgian Federal Science Policy Office
This review provides explanations of how geodesy, rotation and gravity can be addressed using radioscience data of an orbiter around a planet or of the lander on its surface. The planet Mars is the center of the discu...
The knowledge of Martian geology has increased enormously in the last 40 yr. Several missions orbiting or roving Mars have revolutionized our understanding of its evolution and geological features, which in several wa...