he Ministry of Higher Education Malaysia for funding this research under the Fundamental Research Grant Scheme code FRGS/1/2019/STG02/UKM/02/7。
We present Chandra observations of the nearby polar ring galaxy NGC 660 to study its X-ray source population.Based on our analysis,we detected a total of 23 X-ray sources in the 0.5-8 keV band,with luminosities rangin...
We present a detailed analysis of the soft X-ray emission of 3 C 445 using an archival Chandra High Energy Transmission Grating(HETG) spectrum. Highly-ionized H-and He-like Mg, Si and S lines, as well as a resolved ...
supported by the National Natural Science Foundation of China(NSFC,Grant No.11473023);Hunan Provincial Natural Science Foundation(2015JJ3124)
t We present high spatial resolution X-ray spectroscopy of Tycho's supernova remnant (SNR) using observational data from Chandra. The whole remnant was divided into 26 × 27 regions, with each of them covering 20"...
supported by the National Natural Science Foundation of China (NSFC, Grant Nos. 11503002 and 11533002);the "Fundamental Research Funds for the Central Universities"
The ROSAT All-Sky Survey (RASS) represents one of the most complete and sensitive soft X- ray all-sky surveys to date. However, the deficient positional accuracy of the RASS Bright Source Catalog (BSC) and subsequ...
supported by the Research Fund for the Doctoral Program of the Southwest University of Science and Technology (No. 14zx7102)
We study ten galaxy groups and clusters suggested in the literature to be "fossil systems(FSs)"based on Chandra observations. According to the M(500)- T and LX- T relations, the gas properties of FSs are not phy...
Supported by the National Natural Science Foundation of China
We present high spatial resolution X-ray spectroscopy of supernova rem- nant G292.0+1.8 made with Chandra observations. The X-ray emitting region of this remnant was divided into 25 × 25 pixels with a scale of 20" ...
Supported by the National Natural Science Foundation of China(Grant Nos. 10878001, 10973010 and 11125313);the National Basic Research Program of China (973 Program; Grant Nos. 2009CB824900 and 2009CB824904);the Shanghai Science and Technology Commission (Program of Shanghai Subject Chief Scientist; Grant Nos. 12XD1406200 and 11DZ2260700)
We present a study of a fossil cluster,SDSS J0150–1005(z 0.364),with high spatial resolution based on the imaging spectroscopic analysis of Chandra observations.The Chandra X-ray image shows a relaxed and symmetric...
supported by National Natural Science Foundation of China(Grant Nos.10673008,10878001and10973010);the Ministry of Science and Technology of China(Grant No.2009CB824900/2009CB24904);the Ministry of Education of China(the NCET Program)
By analyzing the azimuthal variations of total gravitating mass profiles in the central 300 h^-1 71 kpc regions of four galaxy clusters with Chandra data, we find that the azimuthally-averaged mass profiles may have b...
supported by the National Natural Science Foundation of China(Distinguished Young Scholars,Grant Nos.10425313,10833006 and 10621303);Chinese Academy of Sciences’Hundred Talent Program;973 project of the Ministry of Science and Technology of China(GrantNo.2007CB815406)
We present our initial results from a study of 14 (U)LIRGs with a doublenucleus (z 〈0.15) and an AGN signature in the Chandra archive.The goals of our study are to search for more possible cases of binary AGNs an...