The ATLAS(3D) project - XIX. The hot gas content of early-type galaxies: fast versus slow rotators

The ATLAS(3D) project - XIX. The hot gas content of early-type galaxies: fast versus slow rotators

For early-type galaxies, the ability to sustain a corona of hot, X-ray-emitting gas could have played a key role in quenching their star formation history. A halo of hot gas may act as an effective shield against the acquisition of cold gas and can quickly absorb stellar mass loss material. Yet, sin...

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Bibliografiska uppgifter
Huvudupphovsmän: Sarzi, M, Alatalo, K, Blitz, L, Bois, M, Bournaud, F, Bureau, M, Cappellari, M, Crocker, A, Davies, R, Davis, T, de Zeeuw, P, Duc, P, Emsellem, E, Khochfar, S, Krajnovic, D, Kuntschner, H, Lablanche, P, McDermid, R, Morganti, R, Naab, T, Oosterloo, T, Scott, N, Serra, P, Young, L, Weijmans, A
Materialtyp: Journal article
Språk:English
Publicerad: 2013

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