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 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);Shanghai Jiao Tong University Innovation Fund For Postgraduates
By performing a two dimensional spectral analysis on the galaxy group NGC 533 with high-quality Chandra data, we find that the metal abundance distribution in this group is anisotropic. In the area around 2.5′ from t...
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(Grant Nos.10673008,10878001 and 10973010);the Ministry of Science and Technology of China(Grant No.2009CB824900/2009CB24904);the Ministry of Education of China(the NCET Program)
By analyzing Chandra X-ray data of a sample of 21 galaxy groups and 19 galaxy clusters, we find that in 31 sample systems there exists a significant central (R ≤ 10 h^-171 kpc) gas entropy excess (AK0), which cor...
supported by the National Natural Science Foundation of China (Grant Nos. 10673008,10878001 and 10973010);the Ministry of Science and Technology of China (Grant No. 2009CB824900/2009CB24904);the Ministry of Education of China (the NCET Program)
By creating and analyzing two dimensional gas temperature and abundance maps of the RGH 80 compact galaxy group with high-quality Chandra data,we detect a high-abundance ( 0.7 Z⊙) arc,where the metal abundance is s...
supported by the National Natural Science Foundation of China(Grant Nos.10503008,10673008,10878001 and 10973010);the Ministry of Science and Technology of China(Grant No.2009CB824900/2009CB24904);the Ministry of Education of China(the NCET Program)
We present a high spatial resolution study of metal distributions in the nearby, gas-rich elliptical galaxies NGC 4374 and NGC 4636 with the Chandra ACIS archive data. We define the hardness ratio HRFeL as the ratio o...