supported by the Fundamental Research Funds for the Central Universities,the National Key Research and Development Program of China(Grant No.2020YFC2201500);the National Natural Science Foundation of China(Grant Nos.12147103,11821505,11975236,and 12235008);the Strategic Priority Research Program of the Chinese Academy of Sciences(Grant No.XDB23030100)。
For space-based gravitational wave(GW)detection,the main noise source for massive black hole binaries(MBHBs)is attributed to approximately 107 double white dwarf binaries in the foreground.For a GW source,the amplitud...
We presented the first photometric analysis of the V1961 Cyg and V0890 Lyr binary systems.We observed and analyzed these systems at an observatory in France as part of the Binary Systems of South and North (BSN)Projec...
supported by the Ministry of Science and Education,FEUZ-2020-0038。
The spinning-up of the accreting component in the process of conservative mass exchange is considered in binary systems—progenitors of systems consisting of a main sequence Be-star and an O-subdwarf.During the mass e...
supported by the National Natural Science Foundation of China(under grant Nos.12373044,12273014,12203051,12403035,12393811,12288102,and 12041304);the Natural Science Foundation of Shandong Province(under grant Nos.ZR2023MA050,and ZR2021MA013);the China Postdoctoral Science Foundation(under grant Nos.2024M751375 and 2024T170393);the Postdoctoral Fellowship Program of CPSF(under grant No.GZB20240307);the Jiangsu Funding Program for Excellent Postdoctoral Talent(under grant No.2024ZB705);the Tianshan Talent Program of Xinjiang Uygur autonomous region(under grant No.2023TSYCTD0013);the CAS“Light of West China”Program(under grant No.2018-XBQNXZ-B-022)。
The double neutron star PSR J1846-0513 is discovered by the Five-hundred-meter Aperture Spherical radio Telescope(FAST)in Commensal Radio Astronomy FAST Survey.The pulsar is revealed to be harbored in an eccentric orb...
We conducted the first light curve study of the binary star EL Tuc within the Binary Systems of South and North project's framework.The photometric observations were made using standard multiband BVR_cI_c filters at a...
supported by the National Natural Science Foundation of China(Nos.12288102 and 12333008);the National Key R&D Program of China(No.2021YFA1600403);support from the International Centre of Supernovae,Yunnan Key Laboratory(No.202302AN360001);the Yunnan Revitalization Talent Support Program-Science&Technology Champion Project(No.202305AB350003);the Yunnan Fundamental Research Projects(Nos.202401BC070007 and 202201B C070003);the science research grants from the China Manned Space Project。
A neutron star(NS)has many extreme physical conditions,and one may obtain some important information about an NS via accreting neutron star binary(ANSB)systems.The upcoming Chinese Space Station Telescope(CSST)provide...
the financial support of grant No.075-15-2022-262(13.MNPMU.21.0003)of the Ministry of Science and Higher Education of the Russian Federation。
The results of seventeen years of speckle interferometric monitoring of seven objects(Chara 122Aa,GJ 3010,HIP1987,GJ 3076,HIP 11253,HIP 11352,and HIP 14929)are presented.Observational data were obtained at the 6 m Big...
support by the Astronomical station Vidojevica,funding from the Ministry of Science,Technological Development and Innovation of the Republic of Serbia(contract No.451-03-66/2024-03/200002);by the EC through project BELISSIMA(call FP7-REGPOT-2010-5,No.265772);financed by Silesian University of Technology Statutory Activities grant No.BK-250/RAu-11/2024。
Low mass ratio contact binary systems are more likely to have unstable orbits and potentially merge.In addition,such systems exhibit characteristics such as starspots and high energy emissions(UV)suggestive of chromos...
financial support of the APVV-20-0148,VEGA 2/0030/21 and VEGA 2/0031/22grants;support from the Government Office of the Slovak Republic within EU NextGenerationEU through the Recovery and Resilience Plan for Slovakia under the project No.09I03-03-V01-00002;the private company 4pi Systeme GmbH for partial sponsorship。
In this study,we present an investigation of the newly discovered dwarf nova ASASSN-19oc during its superoutburst on 2019 June 2.We carried out detailed UBVRcIc-photometric observations and also obtained a spectrum on...
support from the SRF INSPIRE(IF 170314)fellowship program,Government of India;financial support from the SERB Core Research Grant project,the Government of India。
Contact binaries at various stages of evolution unveil various operating mechanisms that drive them.We report the photometric and period variation analysis of two contact binaries EV Cnc and AH Cnc in open cluster M67...