Linear structures in the core of the Coma cluster of galaxies.

The hot x-ray-emitting plasma in galaxy clusters is predicted to have turbulent motion, which can contribute around 10% of the cluster's central energy density. We report deep Chandra X-ray Observatory observations of the Coma cluster core, showing the presence of quasi-linear high-density arms...

Полное описание

Библиографические подробности
Главные авторы: Sanders, J, Fabian, A, Churazov, E, Schekochihin, A, Simionescu, A, Walker, SA, Werner, N
Формат: Journal article
Язык:English
Опубликовано: 2013