supported by the National Natural Science Foundation of China (NSFC,12233006);supported by the NSFC 12203042;the Foundations of Yunnan Province 202301AU070009。
The middle-aged Galactic supernova remnant (SNR)-the Cygnus Loop (CL)-displays a peculiar morphology in X-rays,featuring a blowout in the southern region.The underlying process accounting for the formation of the pecu...
supported by the National Key Research and Development Program of China(2021YFA0715101);the National Natural Science Foundation of China(NSFC,grant Nos.12033009 and 12103087);the Strategic Priority Research Program of the Chinese Academy of Sciences(XDA0350300);the International Partnership Program of Chinese Academy of Sciences(020GJHZ2022034FN);the Yunnan Fundamental Research Projects(202201AU070225,202301AT070328,202401AT070141);the Young Talent Project of Yunnan Revitalization Talent Support Program。
High-precision ephemerides not only support space missions,but can also be used to study the origin and future of celestial bodies.In this paper,a coupled orbit-rotation dynamics model that fully takes into account th...
funded by the National Natural Science Foundation of China(NSFC,grant Nos.12363011,52275270,and 52275269);Natural Science Foundation of Xinjiang Uygur Autonomous Region(No.2023D01C22);the Tianchi Talents Program of Xinjiang,the National Key Basic Research Program of China(No.2021YFC2203501);the Xinjiang Postdoctoral Foundation。
Active reflectors are often used to compensate the surface distortion caused by environmental factors that degrade the electromagnetic performance of large high-frequency reflector antennas.This is crucial for maintai...
supported by the National Natural Science Foundation of China(No.12233003);the support from Laboratory of Pinghu,Pinghu,China。
Temporary capture efficiency is studied in the framework of the circular restricted three-body problem in two steps.First, a non-uniform distribution of test particles around the secondary's orbit is obtained by fully...
supported by the National Natural Science Foundation of China(NSFC,grant Nos.12073080,11933010,11921003,12233011,and 12225305)。
AT2021lfa,also known as ZTF21aayokph,was detected by the Zwicky Transient Facility on 2021 May 4,a 05:34:48 UTC.Follow-up observations were conducted using a range of ground-based optical telescopes,as wel as Swift/XR...
Leighton Chajnantor Telescope(LCT), i.e., the former Caltech Submillimeter Observatory telescope, will be refurbished at the new site in Chajnantor Plateau, Chile in 2023. The environment of LCT will change significan...
the National Key Research and Development Program of China under No.2021YFC2203600;the National Natural Science Foundation of China under Nos.52005377 and 52275268;the National Defense Basic Scientific Research Program of China under No.JCKY2021210B007;Wuhu and Xidian University Special Fund for Industry-University-Research Cooperation under No.XWYCXY-012021012;Youth Innovation Team of Shaanxi Universities under No.201926.
Obtaining the wind load distribution on the telescope aperture is very important to estimate its influence and reduce the wind disturbance on the telescope system.The aperture of the radio telescope structure can be a...
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 National Natural Science Foundation of China(NSFC,grant No.12203095);the Youth Innovation Promotion Association,CAS(No.Y202019);Natural Science Foundation of Xinjiang Uygur Autonomous Region(No.2022D01B220);Tianchi Doctoral Program 2021;the Scientific Instrument Developing Project of the Chinese Academy of Sciences(No.PTYQ2022YZZD01).
This paper presents a modified Stewart platform that enables precise adjustment of the sub-reflector for the Qitai Radio Telescope(QTT).QTT demands a parallel platform capable of carrying a heavy load(≥4000 kg),and m...
supported by the National Natural Science Foundation of China(NSFC,Grant Nos.12288102,12090040/1,11873016);the National Key R&D Program of China(Nos.2021YFA1600401 and 2021YFA1600400);the Chinese Academy of Sciences(CAS),the International Centre of Supernovae,Yunnan Key Laboratory(No.202302AN360001);the Yunnan Fundamental Research Projects(grant Nos.202201BC070003,202001AW070007);the“Yunnan Revitalization Talent Support Program”Science&Technology Champion Project(No.202305AB350003);supported by the Klaus Tschira Foundation;by the Deutsche Forschungsgemeinschaft(DFG,German Research Foundation)—Project-ID 138713538—SFB 881(“The Milky Way System”,Subproject A10)。
Type Ia supernovae(SNe Ia)play a key role in the fields of astrophysics and cosmology.It is widely accepted that SNe Ia arise from thermonuclear explosions of white dwarfs(WDs)in binary systems.However,there is no con...