MERGER

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GRB 210323A:Signature of Long-lasting Lifetime of Supra-massive Magnetar as the Central Engine from the Merger of Binary Neutron Star
《Research in Astronomy and Astrophysics》2024年第8期32-41,共10页Yingze Shan Xiaoxuan Liu Xing Yang Haoyu Yuan Houjun Lü 
supported by the Guangxi Science Foundation(grant No.2023GXNSFDA026007);the Program of Bagui Scholars Program(LHJ)。
Theoretically,a supra-massive neutron star or magnetar may be formed after the merger of binary neutron stars.GRB210323A is a short-duration gamma-ray burst(GRB)with a duration of lasting~1 s.The light curve of the pr...
关键词：(stars)gamma-ray burst general-(stars)gamma-ray burst individual(GRB 210323A)-stars MAGNETARS 
FRB 171019:an event of binary neutron star merger?
《Research in Astronomy and Astrophysics》2020年第4期107-114,共8页Jin-Chen Jiang Wei-Yang Wang Rui Luo Shuang Du Xuelei Chen Ke-Jia Lee Ren-Xin Xu 
supported by the Mo ST Grant(2016YFE0100300);the National Key R&D Program of China(2017YFA0402602);NSFC(11633004,11473044,11653003,11673002 and U1531243);the Strategic Priority Research Program of CAS(XDB23010200);the CAS grants(QYZDJSSW-SLH017 and CAS XDB 23040100)。
The fast radio burst,FRB 171019,was relatively bright when discovered first by ASKAP but was identified as a repeater with three faint bursts detected later by GBT and CHIME.These observations lead to the discussion o...
关键词：pulsars:general stars:neutron dense MATTER GRAVITATIONAL waves 
A global analysis searching for neutrinos associated with black hole merger gravitational wave events
《Research in Astronomy and Astrophysics》2018年第11期11-16,共6页Yu-Zi Yang Jia-Jie Ling Wei Wang Zhao-Kan Cheng 
funded by the National Natural Science Foundation of China (Grant No. 11080922)
Several neutrino observatories have searched for coincident neutrino signals associated with gravitational waves induced by the merging of two black holes. No statistically significant neutrino signal in excess of the...
关键词：gravitational wave black hole merger neutrino fluence global analysis 
An axion-like scalar field environment effect on binary black hole merger
《Research in Astronomy and Astrophysics》2018年第6期35-48,共14页Qing Yang Li-Wei Ji Bin Hu Zhou-Jian Cao Rong-Gen Cai 
supported by Beijing Normal University (Grant No. 312232102);partially supported by the Chinese National Youth Thousand Talents Program;the Fundamental Research Funds for the Central Universities (Grant No. 310421107);supported in part by the National Natural Science Foundation of China (Grant Nos. 11690022, 11375247, 11435006 and 11647601);by the Strategic Priority Research Program of CAS (Grant No. XDB23030100);by the Key Research Program of Frontier Sciences of CAS
The environment, such as an accretion disk, could modify the signal of the gravitational wave from astrophysical black hole binaries. In this article, we model the matter field around intermediatemass binary black hol...
关键词：stars: black holes gravitational waves methods: numerical 
Multi-transition study of the peculiar merger Arp 299
《Research in Astronomy and Astrophysics》2017年第8期1-12,共12页Qian Jiao Ming Zhu 
supported by the China Ministry of Science and Technology under the State Key Development Program for Basic Research (2012CB821800);supported by the Joint Research Fund in Astronomy (U1531246) under cooperative agreement between the National Natural Science Foundation of China (NSFC) and the Chinese Academy of Sciences (CAS);supported by the Strategic Priority Research Program “The Emergence of Cosmological Structures” of the Chinese Academy of Sciences (Grant No. XDB09000000)
We present a multi-transition study to investigate the physical properties of dust and molecular gas in the archetypical merger Arp 299 by using data including James Clerk Maxwell Telescope(JCMT)850 and 450 μm observ...
关键词：GALAXIES merge — galaxies Arp 299 — galaxies dust — galaxies molecular gas — galaxies warm center 
The Evolution of Advanced Merger (U)LIRGs on the Color-Stellar Mass Diagram被引量：1
《Research in Astronomy and Astrophysics》2016年第8期89-94,共6页Rui Guo Cai-Na Hao Xiao-Yang Xia 
supported by the National Natural Science Foundation of China(Grant Nos11373027,10973011 and 11003015);sponsored by SRF for ROCS, SEM
Based on a sample of 79 local advanced merger （adv-merger） （U）LIRGs, we search for evidence of quenching processes by investigating the distributions of star formation history indicators （EW（Ha）, EW（HfiA） and...
关键词：galaxies： evolution -- galaxies formation -- galaxies interactions -- galaxies starburst -- infrared： galaxies 
Observational evidence for the evolution of nuclear metallicity and star formation rate with the merger stage
《Research in Astronomy and Astrophysics》2016年第7期113-124,共12页Rui Guo Cai-Na Hao Xiao-Yang Xia Peng Wei Xin Guo 
supported by the National Natural Science Foundation of China(Grant Nos.11373027 and11003015);SRF for ROCS,SEM.Funding for the creation and distribution of the SDSS Archive has been provided by the Alfred P.Sloan Foundation,the Participating Institutions,the National Aeronautics and Space Administration,the National Science Foundation,the U.S.Department of Energy,the Japanese Monbukagakusho,and the Max Planck Society
We investigate the evolution of nuclear gas-phase oxygen abundance and star formation rate（SFR） of local far-infrared selected star-forming galaxies along the merger sequence, as traced by their optical morphologies...
关键词：GALAXIES abundances galaxies evolution galaxies interactions galaxies starburst galaxies star formation infrared GALAXIES 
Contribution of dust produced by binary merger ejecta
《Research in Astronomy and Astrophysics》2015年第1期55-63,共9页Zhao-Jun Wang Chun-Hua Zhu Guo-Liang Lü 
Supported by the National Natural Science Foundation of China
By means of a population synthesis code and by constructing a simple toy model of dust produced by asymptotic giant branch（AGB） stars, common envelope（CE） ejecta and binary merger ejecta, we estimate the dust prod...
关键词：binaries： close stars： evolution circumstellar matter DUST 
A multiwavelength view of the ISM in the merger remnant galaxy Fornax A
《Research in Astronomy and Astrophysics》2013年第8期885-898,共14页Swati Pralhadrao Deshmukh Bhagorao Tukaram Tate Nilkanth Dattatray Vagshette Sheo Kumar Pandey Madhav Khushalrao Patil 
supported by UGC, New Delhi under the major research project F.No. (36-240/2008-SR);the use of the High Performance Computing Facility developed under the DST- FIST scheme sanction No. SR/FST/PSI-145
We present multi-wavelength imagery of the merger remnant galaxy NGC 1316 with an objective to study the dust content and its association with the other phases of the interstellar medium. Color-index maps as well as e...
关键词：GALAXIES individual （NGC 1316） - galaxies： ISM - X-rays： ISM - （ISM：） dust - extinction - galaxies： elliptical and lenticular  cD 
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