supported by the National Key R&D Program of China(2021YFC2203502 and 2022YFF0711502);the National Natural Science Foundation of China(NSFC)(12173077);the Tianshan Talent Project of Xinjiang Uygur Autonomous Region(2022TSYCCX0095 and 2023TSYCCX0112);the Scientific Instrument Developing Project of the Chinese Academy of Sciences(PTYQ2022YZZD01);China National Astronomical Data Center(NADC);the Operation,Maintenance and Upgrading Fund for Astronomical Telescopes and Facility Instruments,budgeted from the Ministry of Finance of China(MOF)and administrated by the Chinese Academy of Sciences;Natural Science Foundation of Xinjiang Uygur Autonomous Region(2022D01A360).
Astronomical spectroscopy is crucial for exploring the physical properties,chemical composition,and kinematic behavior of celestial objects.With continuous advancements in observational technology,astronomical spectro...
supported by the National Key R&D Program of China(Grant No.2023YFA1608000);the National Natural Science Foundation of China(NSFC)(Grant Nos.12003045,and 12173013);the Science Foundation of Hebei Normal University(Grant No.L2022B07);the project of Hebei Provincial Department of Science and Technology(Grant No.226Z7604G);the Hebei Natural Science Foundation(NSF)(Grant Nos.A2021205006,and A2023205036)。
The Taurus region is one of the most extensively studied star-forming regions(SFRs).Surveys indicate that the young stars in this region are comprised of young stellar objects(YSOs)that cluster in groups associated wi...
funded by Taif University,Saudi Arabia,Project No.(TU-DSPP-2024-33)。
Theβ-decay properties of^(67-80)As nuclei have been investigated within the framework of the proton-neutron quasi-particle random phase approximation(pn-QRPA)model.The nuclear deformation obtained from the finite ran...
supported in part by the National Natural Science Foundation of China(Grant Nos.12004279,92476113 and 12074283);by City University of Hong Kong(Project No.9610522);the General Research Fund from Hong Kong Research Grants Council(Nos.11315822,11301624);Joint NSFC/RGC Collaborative Research Scheme(No.CRS_CityU103/24).
Hanbury-Brown and Twiss(HBT)effect is the foundation for stellar intensity interferometry.However,it is a phase insensitive two-photon interference effect.Here we extend the HBT interferometer by mixing intensity-matc...
The October edition of FaW TOKYO,held at Tokyo Big Sight,Japan,concluded on a high note,uniting 892 exhibitors from 28 countries and attracting 21,247 visitors from 48 countries,marking another successful gathering of...
supported by the National Natural Science Foundation of China(12261141689,12273075,and 12373108);the National Key R&D Program of China No.2019YFA0405502;the science research grants from the China Manned Space Project with No.CMS-CSST-2021-B05。
Stellar classification and radius estimation are crucial for understanding the structure of the Universe and stella evolution.With the advent of the era of astronomical big data,multimodal data are available and theor...
One of the most important goals of modern cosmology is to understand how galaxies form and evolve in ecosystems defined by the cosmic density field. The formation of galaxies is a process through which cold baryonic g...
supported by the National Key Research and Development Program of China(Grant No.2022YFA1602902);the National Natural Science Foundation of China(Grant Nos.12073002,12233001,and 8200906879);the China Manned Space Project。
As a major interstellar medium,the atomic neutral hydrogen(H_(I))plays an important role in the galaxy evolution.It provides the ingredient for star formation,and sensitively traces the internal processes and external...