SDSS-IV MaNGA: the different quenching histories of fast and slow rotators

Do the theorised different formation mechanisms of fast and slow rotators produce an observable difference in their star formation histories? To study this we identify quenching slow rotators in the MaNGA sample by selecting those which lie below the star forming sequence and identify a sample of qu...

Mô tả đầy đủ

Chi tiết về thư mục
Những tác giả chính: Smethurst, RJ, Masters, KL, Lintott, CJ, Weijmans, A, Merrifield, M, Penny, SJ, Aragón-Salamanca, A, Brownstein, J, Bundy, K, Drory, N, Law, DR, Nichol, RC
Định dạng: Journal article
Được phát hành: Oxford University Press 2017

Những quyển sách tương tự