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University of Central Lancashire

Dust in Early-Type Galaxies using Herschel-ATLAS and GAMA data

Abstract

dc:description.abstract

This work investigates the properties of Early-Type Galaxies (ETGs; elliptical and lenticulars) containing thermal dust emission, with aims of linking the formation and evolution of these galaxies with their current dust properties. Three different proxies for morphology are considered for selecting ETGs, and these are tested against three sets of visually classified galaxies. We find that classifying ETGs as those galaxies in the optical Red Sequence results in samples with

Degree

thesis:*
Name dc:type.qualificationname
phd
Level dc:type.qualificationlevel
doctoral
Grantor dc:publisher.institution
University of Central Lancashire
Year dc:date.issued
2014

Author and committee

dc:creator, dc:contributor.*
Author dc:creator
  • Agius, Nicola Kristina

Subjects

dc:subject × 2

Rights

Language dc:language
en

Chain of custody

source
Harvested from
University of Central Lancashire
Base URL
clok.uclan.ac.uk/cgi/oai2
Last updated
2026-07-24
Source record
OAI-PMH GetRecord
citation

Agius, Nicola Kristina. Dust in Early-Type Galaxies using Herschel-ATLAS and GAMA data. doctoral thesis, University of Central Lancashire, 2014.