云南高校图书馆联盟文献共享服务平台- SUPERNOVA

SUPERNOVA: 作品数：148被引量：36H指数：3; 导出分析报告; 相关领域：天文地球更多>>; 相关作者：洪碧海李小波申虹王祥玉更多>>; 相关机构：南京大学深圳市与函设计工作室惠而浦(中国)股份有限公司移动信息图库更多>>; 相关期刊：更多>>; 相关基金：国家自然科学基金国家重点基础研究发展计划以色列科学基金更多>>

Pulsar scintillation reveals the Gum Nebula as a scattering screen: 《Science China(Physics,Mechanics & Astronomy)》2025年第3期192-192,共1页Dan Stinebring; Since soon after the discovery of radio pulsars in 1968,their scintillation due to multi-path scattering in the interstellar medium(ISM)emerged as a useful tool in studying the ISM.For example,a recent study with the ...; 关键词：SCATTERING SUPERNOVA pulsar

Forecasting supernova observations with the CSST:I.Photometric samples: 《Science China(Physics,Mechanics & Astronomy)》2024年第11期164-177,共14页Chengqi Liu Youhua Xu Xianmin Meng Xin Zhang Shi-Yu Li Yuming Fu Xiaofeng Wang Shufei Liu Zun Luo Guanghuan Wang Hu Zhan; supported by the National Key R&D Program of China(Grant Nos.2022YFF0503400 and 2022YFF0503401);China Manned Space Program(Grant Nos.CMS-CSST-2021-B01,CMS-CSST-2021-B04,and CMS-CSST2021-A12);Science Program of Beijing Academy of Science and Technology(Grant No.24CD014);National Natural Science Foundation of China(Grant Nos.12288102 and 12033003);Tencent Xplorer Prize。; The China Space Station Telescope(CSST,also known as Xuntian)is a serviceable two-meter-aperture wide-field telescope operating in the same orbit as the China Space Station.The CSST plans to survey a sky area of 17,50...; 关键词：space-based ultraviolet optical and infrared telescopes SUPERNOVAE data analysis

Pasta Phases in Dense Matter: 《原子核物理评论》2024年第3期811-817,共7页SHEN Hong HU Jinniu JI Fan WU Xuhao JU Min; 国家自然科学基金资助项目(12175109)。; The pasta phases are expected to appear in hot supernova matter and cold neutron stars.In supernova matter,the pasta phases with a series of geometric shapes are studied using the compressible liquid-drop(CLD)model,wh...; 关键词：pasta phase supernova matter neutron star

The Energy Sources and the Explosion Mechanism of Ca-rich Supernova PTF 10iuv: 《Research in Astronomy and Astrophysics》2024年第9期106-118,共13页Qiu-Ping Huang Shan-Qin Wang Tao Wang Wen-Pei Gan Deng-Wang Shi Liu-Yi Wang En-Wei Liang; supported by National Natural Science Foundation of China(NSFC,grant Nos.11963001,12133003,11833003,11973020(C0035736),and U1938201);supported by the Guangxi Talent Program(“Highland of Innovation Talents”)。; In this paper,we perform the detailed modeling for the light curves(LCs)of PTF 10iuv which is a calcium-rich(Ca-rich)supernova(SN)to constrain the physical properties of its ejecta and the energy sources,as well as th...; 关键词：(stars:)supernovae:general (stars:)supernovae:individual(PTF 10iuv) (stars:)novae cataclysmic variables

Swift XRT Analysis of Type II-P Supernova SN 2008ij: 《International Journal of Astronomy and Astrophysics》2024年第3期220-229,共10页SH. M. Shehata Ahmed M. Fouad R. M. Samir A. A. Shaker; This study investigates the X-ray properties and evolution of Type II supernovae (SNe II) observed by Swift, examining variations among supernovae and exploring their X-ray characteristics over time. We present the fi...; 关键词：X-Ray Core Collapse Supernova Swift (XRT) Observations

Detecting neutrinos from supernova bursts in PandaX-4T: 《Chinese Physics C》2024年第7期14-21,共8页庞彬宇阿布都沙拉木·阿布都克力木薄子豪陈葳谌勋程晨成兆侃崔祥仪樊英杰方德清符长波付孟婷耿立升 Karl Giboni 顾琳慧郭绪元韩晨成韩柯何昶达何金荣黄迪黄彦霖黄俊挺黄周侯汝全侯钰季向东巨永林李晨翔李家富李名川李帅杰李涛林箐刘江来陆聪聪芦晓盈罗棱尹罗云阳马文博马余刚冒亚军孟月宁旭阳祁宁春钱志成任祥祥 Nasir Shaheed 尚晓凤邵熙元申国防司琳孙文良谈安迪陶奕王安庆王萌王秋红王少博王思广王为王秀丽王舟魏月环武蒙蒙邬维浩夏经铠肖梦姣肖翔谢鹏伟燕斌斌颜玺雨杨继军杨勇姚玉坤喻纯旭袁影苑哲鑫宁张丹张敏桢张鹏张世博张澍张涛张洋张瀛心张园园赵力郑其斌周济芳周宁周小朋周永周钰博; the National Natural Science Foundation of China(12090060,12090063,12105052,12005131,11905128,11925502);the Office of Science and Technology,Shanghai Municipal Government,China(22JC1410100)。; Neutrinos from core-collapse supernovae are essential for understanding neutrino physics and stellar evolution.Dual-phase xenon dark matter detectors can be used to track explosions of galactic supernovae by detecting...; 关键词：core-collapse supernovae NEUTRINOS liquid xenon detectors supernova early warnings

Supernova 1987A's Keyhole:A Long-lived Jet-pair in the Final Explosion Phase of Core-collapse Supernovae: 《Research in Astronomy and Astrophysics》2024年第7期89-94,共6页Noam Soker; the Pazy Foundation supported this research。; I further study the manner by which a pair of opposite jets shape the“keyhole”morphological structure of the core-collapse supernova(CCSN)SN 1997A,now the CCSN remnant(CCSNR)1987A.By doing so,I strengthen the claim ...; 关键词：STARS massive-(stars)supernovae general-(stars)supernovae individual(SN 1987A)-ISM supernova remnants-stars jets

Gravitational Waves Background, as Well as Some UFO, FRB and Supernova Flares, Are Due to Compressibility of the Spacetime (CoST): 《Journal of High Energy Physics, Gravitation and Cosmology》2024年第1期67-70,共4页Evgeny A. Novikov; The recently observed gravitational wave background is explained in terms of the quantum modification of the general relativity (Qmoger). Some UFO, FRB and supernova flares also can be explained in terms of Qmoger.; 关键词：Gravitational Wave Background Quantum Modification of the General Relativity Compressibility of the Spacetime (CoST)

Point-symmetry in SNR G1.9+0.3:A Supernova that Destroyed its Planetary Nebula Progenitor: 《Research in Astronomy and Astrophysics》2024年第1期165-172,共8页Noam Soker; supported by a grant from the Israel Science Foundation(769/20)。; I analyze a new X-ray image of the youngest supernova remnant(SNR)in the Galaxy,which is the type Ia SNR G1.9+0.3,and reveal a very clear point-symmetrical structure.Since explosion models of type Ia supernovae(SNe Ia...; 关键词：(stars:)supernovae:general ISM:supernova remnants (stars:)binaries(including multiple):close (ISM:)planetary nebulae:general stars:jets

The dusty and extremely red progenitor of the typeⅡsupernova 2023ixf in Messier 101: 《Science China(Physics,Mechanics & Astronomy)》2024年第1期160-172,共13页Danfeng Xiang Jun Mo Lingzhi Wang Xiaofeng Wang Jujia Zhang Han Lin Lifan Wang; supported by the National Natural Science Foundation of China(Grant Nos.12288102,12033003,and 11633002);the Ma Huateng Foundation;the Scholar Program of Beijing Academy of Science and Technology(Grant No.DZ:BS202002);the Tencent Xplorer Prize;sponsored(in part)by the Chinese Academy of Sciences(CAS);through a grant to the CAS South America Center for Astronomy(CASSACA)in Santiago,Chile;Funding for the LJT has been provided by the CAS and the People’s Government of Yunnan Province。; Stars with initial masses in the range of 8-25 solar masses are thought to end their lives as hydrogen-rich supernovae(SNeⅡ).Based on the pre-explosion images of Hubble space telescope(HST)and Spitzer space telescope...; 关键词：stellar evolution mass loss red supergiants infrared emission SUPERNOVAE

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