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Unravelling the origins of S0 galaxies using maximum likelihood analysis of planetary nebulae kinematics The origins of S0s from PN kinematics (2011)

First Author: Cortesi A

Attributed to: Nottingham Astronomy Rolling Grant 2011 - 2016 funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1111/j.1365-2966.2011.18429.x

Publication URI: http://dx.doi.org/10.1111/j.1365-2966.2011.18429.x

Type: Journal Article/Review

Parent Publication: Monthly Notices of the Royal Astronomical Society

Issue: 1