The Structure and Kinematics of Little Blue Spheroid Galaxies

GAMA Survey Team, SAMI Survey Team

Research output: Contribution to conferenceAbstract

Abstract

A population of blue, morphologically early-type galaxies, dubbed "Little Blue Spheroids" (LBSs), has been identified as a significant contributor to the low redshift galaxy population in the GAMA survey. Using deep, high-resolution optical imaging from KiDS and the new Bayesian, two-dimensional galaxy profile modelling code PROFIT, we examine the detailed structural characteristics of LBSs, including low surface brightness components not detected in previous SDSS imaging. We find that these LBS galaxies combine features typical of early-type and late-type populations, with structural properties similar to other low- mass early types and star formation rates similar to low-mass late types. We further consider the environments and SAMI-derived IFU kinematics of LBSs in order to investigate the conditions of their formation and the current state of their dynamical evolution.
Original languageEnglish
Publication statusPublished - 2018
Event231st American Astronomical Society Meeting - Gaylord National Resort & Convention Center, Washington, United States
Duration: 8 Jan 201812 Jan 2018
Conference number: 231

Conference

Conference231st American Astronomical Society Meeting
Abbreviated titleAAS
CountryUnited States
CityWashington
Period8/01/1812/01/18

Fingerprint Dive into the research topics of 'The Structure and Kinematics of Little Blue Spheroid Galaxies'. Together they form a unique fingerprint.

  • Cite this

    GAMA Survey Team, & SAMI Survey Team (2018). The Structure and Kinematics of Little Blue Spheroid Galaxies. Abstract from 231st American Astronomical Society Meeting, Washington, United States. https://ui.adsabs.harvard.edu/abs/2018AAS...23114945M