《Research in Astronomy and Astrophysics》

作品数：2959被引量：1282H指数：14
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《Research in Astronomy and Astrophysics》
主办单位：Chinese Astronomical Society;National Astronomical Observatories;Chinese Academy of Sciences
最新期次：2024年12期更多>>
发文主题：STARSGALAXIESSUNBINARIESMETHODS更多>>
发文领域：天文地球理学自动化与计算机技术航空宇航科学技术更多>>
发文作者：须重明钟钊新翟迪生杨兰田徐燕侯更多>>
发文机构：中国科学院国家天文台北京师范大学中国科学技术大学中国科学院云南天文台更多>>
发文基金：国家自然科学基金国家重点基础研究发展计划中国博士后科学基金俄罗斯基础研究基金更多>>
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Simulating the Peculiar Periphery of the Cygnus Loop
《Research in Astronomy and Astrophysics》2024年第12期192-206,共15页Jun-Yu Shen Bi-Wen Bao Li Zhang 
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...
关键词：hydrodynamics-methods numerical-ISM supernova remnants 
Multi-layer Perceptron for Predicting Galaxy Parameters(MLP-GaP): Stellar Masses and Star Formation Rates
《Research in Astronomy and Astrophysics》2024年第12期207-218,共12页Xiaotong Guo Guanwen Fang Haicheng Feng Rui Zhang 
support of the National Nature Science Foundation of China (Nos.12303017,and12203096);supported by Anhui Provincial Natural Science Foundation project No.2308085QA33;supported by the science research grants from the China Manned Space Project。
The large-scale imaging survey will produce massive photometric data in multi-bands for billions of galaxies.Defining strategies to quickly and efficiently extract useful physical information from this data is mandato...
关键词：METHODS data analysis-galaxies fundamental parameters-galaxies star formation 
A Real-time Monitor for TeV Gamma-Ray Flare with the LHAASO-WCDA Detector
《Research in Astronomy and Astrophysics》2024年第12期219-228,共10页G.M.Xiang M.Zha J.N.Zhou Y.Xing 
supported in China by NSFC grant No.12393853;the Department of Science and Technology of Sichuan Province China with grant No.24NSFSC0449;NSFC grant No.U2031205。
With its high duty cycle, wide field of view and high detection sensitivity, Water Chereknov Detector Array as one of sub-arrays of Large High Altitude Air Shower Observatory is a promising facility to monitor transie...
关键词：METHODS data analysis-methods observational-gamma-rays galaxies 
Measuring the Time Variation of the Fine-structure Constant with Quasars Detected by LAMOST
《Research in Astronomy and Astrophysics》2024年第12期229-235,共7页Jin-Nan Wei Rui-jie Chen Jun-Jie Wei Martín López-Corredoira Xue-Feng Wu 
supported by the National Natural Science Foundation of China(grant Nos.12422307,12373053,and 12321003);the Key Research Program of Frontier Sciences(grant No.ZDBS-LY-7014);Chinese Academy of Sciences,and the Natural Science Foundation of Jiangsu Province(grant No.BK20221562);supported by the Chinese Academy of Sciences President's International Fellowship Initiative(grant No.2023VMB0001)。
The[O iii]λλ4960,5008 emission lines in the optical spectra of galaxies and quasars have been widely used to investigate the possible variation of the fine-structure constantαover cosmic time.In this work,we utiliz...
关键词：atomic data-(galaxies) QUASARS emission lines-surveys-cosmology observations 
Research in Astronomy and Astrophysics Vol.24 2024 CONTENTS
《Research in Astronomy and Astrophysics》2024年第12期I0001-I0010,共10页
Instructions for authors
《Research in Astronomy and Astrophysics》2024年第12期F0003-F0003,共1页无 
Research in Astronomy and Astrophysics publishes original research papers and reviews on all branches of astronomy and astrophysics.Reviews are by invitation only.Important new results that require rapid publication c...
关键词：submitted RESTRICTED ASTRONOMY 
A Photometric and Astrometric Study of Open Star Clusters FSR-163 and Majaess 215 Using Gaia DR3
《Research in Astronomy and Astrophysics》2024年第12期69-78,共10页Ola Ali A.L.Tadross A.I.Osman Z.M.Hayman 
We have examined most of the astrophysical properties of the two star clusters, FSR-163 and Majaess 215, using the third data release of the Gaia space mission(Gaia DR3). We utilized the py UPMASK method to allocate t...
关键词：(Galaxy) open clusters and associations individual(FSR-163 and Majaess 215)-proper motions-stars luminosity function-mass function-catalogs-Astronomical Databases 
ALMA and GMRT Studies of Dust Continuum Emission and Spectral Lines Toward Oort Cloud Comet C/2022 E3(ZTF)
《Research in Astronomy and Astrophysics》2024年第12期79-90,共12页Arijit Manna Sabyasachi Pal Sekhar Sinha Sushanta Kumar Mondal 
The atomic and molecular compounds of cometary ices serve as valuable knowledge into the chemical and physical properties of the outer solar nebula, where comets are formed. From the cometary atmospheres, the atoms an...
关键词：comets general-planets and satellites composition-radio continuum planetary systems-submillimeter planetary systems-astrochemistry 
High-resolution Observations of Clustered Dynamic Extreme-Ultraviolet Bright Tadpoles Near the Footpoints of Corona Loops
《Research in Astronomy and Astrophysics》2024年第12期91-104,共14页Rui Wang Ying D.Liu L.P.Chitta Huidong Hu Xiaowei Zhao 
supported by National Key R&D Program of China Nos. 2022YFF0503800 and 2021YFA0718600;the Strategic Priority Research Program of the Chinese Academy of Sciences (No. XDB0560000);National Natural Science Foundation of China (NSFC, Grant Nos. 12073032, 42274201, 42150105, and 42204176);the Specialized Research Fund for State Key Laboratories of China。
An extreme ultraviolet(EUV) close-up view of the Sun offers unprecedented detail of heating events in the solar corona. Enhanced temporal and spatial images obtained by the Solar Orbiter during its first science perih...
关键词：SUN activity-Sun atmosphere-Sun corona-Sun transition region Online material Materials only available in the online version of record ANIMATIONS 
Components and Anisotropy of 3D QFP Waves During the Early Solar Eruption
《Research in Astronomy and Astrophysics》2024年第12期105-115,共11页Jialiang Hu Jing Ye Yuhao Chen Zhixing Mei Shanshan Xu Jun Lin 
supported by Strategic Priority Research Program of the Chinese Academy of Sciences No. XDB0560000;National Key R&D Program of China No. 2022YFF0503804;NSFC grants 11933009, 12273107, U2031141 and 12073073;grants associated with the Yunling Scholar Project of Yunnan Province;the Yunnan Province Scientist Workshop of Solar Physics;the Yunnan Key Laboratory of Solar Physics and Space Exploration of Code 202205AG070009;the Special Project for the construction of science and technology innovation centers faced to South Asiaand Southeast Asia-Yunnan International Joint Innovation Platform: “China-Malaysia HF-VHF Advanced Radio Astronomy Technology International Joint Laboratory of Yunnan” (202303AP140003);the support by grants associated with the Yunnan Revitalization Talent Support Program;the Foundation of the Chinese Academy of Sciences (Light of West China Program)。
The propagation of disturbances in the solar atmosphere is inherently three-dimensional(3D), yet comprehensive studies on the spatial structure and dynamics of 3D wave fronts are scarce. Here we conduct high-resolutio...
关键词：SUN corona-Sun coronal mass ejections(CMEs)-shock waves 
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