Stellar angular momentum distribution sets galaxy morphology

Sarah M. Sweet, Karl Glazebrook, Danail Obreschkow, Deanne B. Fisher, Andreas Burkert, Claudia D. P. Lagos, Juan M. Espejo Salcedo

Research output: Contribution to conferencePosterpeer-review

Abstract

The internal distribution of a galaxy's spatially-resolved stellar specific angular momentum is a physically-grounded tracer of its photometric morphology.
Original languageEnglish
Pages13
DOIs
Publication statusPublished - 1 Nov 2019
EventThe Art of Measuring Galaxy Physical Properties - Milano, Italy
Duration: 18 Nov 201922 Nov 2019

Conference

ConferenceThe Art of Measuring Galaxy Physical Properties
Country/TerritoryItaly
CityMilano
Period18/11/1922/11/19

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