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The Possibility of Detecting our Solar System through Astrometry
《Research in Astronomy and Astrophysics》2023年第11期198-204,共7页Dong-Hong Wu 
supported by the National Natural Science Foundation of China(NSFC)(grant No.12103003);the Doctoral research start-up funding of Anhui Normal University。
Searching for exoplanets with different methods has always been the focus of astronomers over the past few years.Among multiple planet detection techniques,astrometry stands out for its capability to accurately determ...
关键词：ASTROMETRY planets and satellites:detection Planetary Systems 
Possibility of Searching for Accreting White Dwarfs with the Chinese Space Station Telescope
《Research in Astronomy and Astrophysics》2022年第5期21-27,共7页Wei Xie Hai-Liang Chen 
partially supported by the National Natural Science Foundation of China(grant Nos.12073071 and 11733008);Yunnan Fundamental Research Projects(grant Nos.202001AT070058 and 202101AW070003);the science research grants from the China Manned Space Project with No.CMS-CSST-2021-A10;Youth Innovation Promotion Association of Chinese Academy of Sciences(grant No.2018076)。
Accreting WDs are very important for the studies of binary evolution,binary population synthesis and accretion physics.So far,there are a lot of accreting WD binaries with low accretion rates,such as cataclysmic varia...
关键词：white dwarf stars whitedwarfs-binarystars close binarystars-low massstars low-massstar 
On the possibility of disk-fed formation in supergiant high-mass X-ray binaries
《Research in Astronomy and Astrophysics》2019年第1期123-130,共8页Ali Taani Shigeyuki Karino Liming Song Mashhoor Al-Wardat Awni Khasawneh Mohammad K.Mardini 
the Abdul Hamed Shoman Foundation (Grant No. 6/2017) for supporting this project;supported by the JSPS KAKENHI (Grant No. 18K03706);supported by the National Key R&D Program of China (2016YFA0400801);the National Natural Science Foundation of China (Grant No. U1838201)
We consider the existence of a neutron star magnetic field by the detected cyclotron lines. We collected data on nine sources of high-mass X-ray binaries with supergiant companions as a test case for our model, to dem...
关键词：binaries:X-rays stars:neutron stars:fundamental parameters ACCRETION DISKS FORMATION magnetic fields 
Possibility of measuring spin precession of the nearest supermassive black hole by using S stars
《Research in Astronomy and Astrophysics》2014年第11期1415-1422,共8页Wen-Biao Han 
Supported by the National Natural Science Foundation of China
The supermassive black hole （SMBH） with a mass of 4 million M⊙ inside the radio source Sgr A＊ in our Galactic center is the nearest SMBH. Once S stars with a shorter period are observed, relativistic precessions e...
关键词：black hole physics -- Galaxy center -- relativity 
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