activity
20082014
most citedChandra Survey of Nearby Highly Inclined Disc Galaxies - III: Comparison with Hydrodynamical Simulations of Circumgalactic Coronae

39 citations · 39 across the 1 of their papers we have counts for

collaborators

8 papers

astro-ph.CO2014★ 39 cited

Chandra Survey of Nearby Highly Inclined Disc Galaxies - III: Comparison with Hydrodynamical Simulations of Circumgalactic Coronae

Jiang-Tao Li, Robert A. Crain, Q. Daniel Wang

X-ray observations of circumgalactic coronae provide a valuable means by which to test galaxy formation theories. Two primary mechanisms are thought to be responsible for the estab…

astro-ph.CO2013

Chandra Survey of Nearby Highly Inclined Disc Galaxies - II: Correlation Analysis of Galactic Coronal Properties

Jiang-Tao Li, Q. Daniel Wang

X-ray observations provide a key tool for exploring the properties of galactic coronae and their formation processes. In an earlier paper, we have presented a Chandra data analysis…

astro-ph.CO2012

Chandra Survey of Nearby Highly-Inclined Disk Galaxies I: X-ray Measurements of Galactic Coronae

Jiang-Tao Li, Q. Daniel Wang

We present a systematical analysis of the Chandra observations of 53 nearby highly-inclined (i>60 degree) disk galaxies to study the coronae around them. This sample covers a broad…

astro-ph.HE2012

Giant H II Regions in M101. I. X-ray Analysis of Hot Gas

Wei Sun, Yang Chen, Li Feng +4

We performed a Chandra X-ray study of three giant H II regions (GHRs), NGC 5461, NGC 5462, and NGC 5471, in the spiral galaxy M101. The X-ray spectra of the three GHRs all contain…

astro-ph.CO2012

Chandra Survey of Nearby Edge-on Disk Galaxies I: Luminosities of Galactic Coronae

Jiang-Tao Li, Q. Daniel Wang

X-ray-emitting coronae of nearby galaxies are expected to be produced either by accretion from the intergalactic medium and/or by various galactic feedback. We herein present a sys…

astro-ph.CO2011

Dynamic S0 Galaxies II: the Role of Diffuse Hot Gas

Jiang-Tao Li, Q. Daniel Wang, Zhiyuan Li +1

Gas loss is thought to be important in SF quenching and morphological transition during the evolution of S0 galaxies. In high density environments, gas loss can be achieved via man…