R
Rongxin Luo
Researcher at University of Alabama in Huntsville
Publications - 3
Citations - 19
Rongxin Luo is an academic researcher from University of Alabama in Huntsville. The author has contributed to research in topics: Intracluster medium & Luminosity. The author has an hindex of 1, co-authored 3 publications receiving 5 citations.
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Journal ArticleDOI
An H α/X-ray orphan cloud as a signpost of intracluster medium clumping
Chong Ge,Rongxin Luo,Ming Sun,Masafumi Yagi,P. Jáchym,Alessandro Boselli,Matteo Fossati,Paul Nulsen,Craig L. Sarazin,Tim Edge,Giuseppe Gavazzi,Massimo Gaspari,Massimo Gaspari,Jin Koda,Yutaka Komiyama,Michitoshi Yoshida +15 more
TL;DR: In this paper, the authors presented the discovery of the first and still the only known isolated cloud (or orphan cloud, OC) detected in both X-rays and H$\alpha$ in the nearby cluster Abell 1367.
Posted Content
Tales of tails: H$\alpha$--X-ray correlation.
Ming Sun,Chong Ge,Rongxin Luo,Masafumi Yagi,Pavel Jáchym,Alessandro Boselli,Matteo Fossati,Paul Nulsen,Michitoshi Yoshida,Giuseppe Gavazzi +9 more
TL;DR: In this paper, a strong linear correlation between the X-ray surface brightness and the H$\alpha$ surface brightness of the diffuse gas in the RPS tails at 10 kpc scales was found.
Journal ArticleDOI
The BIG X-ray tail
Chong Ge,Ming Sun,Masafumi Yagi,Matteo Fossati,Matteo Fossati,William R. Forman,P. Jáchym,Eugene Churazov,Irina Zhuravleva,Alessandro Boselli,Christine Jones,Li Ji,Rongxin Luo +12 more
TL;DR: The Blue Infalling Group (BIG) is a star-bursting compact group with a long H$\alpha$ trail behind it as mentioned in this paper, and the total hot gas mass in the tail is estimated to be approximately 7\times 10^{10} ) with an X-ray bolometric luminosity of 3.8\times 1.8 ǫ s$ −1.