A4 Vertaisarvioitu artikkeli konferenssijulkaisussa
Kinematically Decoupled Cores in Dwarf (Elliptical) Galaxies
Tekijät: Toloba E, Peletier RF, Guhathakurta P, van de Ven G, Boissier S, Boselli A, den Brok M, Falcon-Barroso J, Hensler G, Janz J, Laurikainen E, Lisker T, Paudel S, Rys A, Salo H
Toimittaja: Iodice E, Corsini EM
Konferenssin vakiintunut nimi: International Conference on Multi-Spin Galaxies
Julkaisuvuosi: 2014
Journal: Astronomical Society of the Pacific Conference Series
Kokoomateoksen nimi: Multi-spin galaxies
Tietokannassa oleva lehden nimi: MULTI-SPIN GALAXIES
Lehden akronyymi: ASTR SOC P
Sarjan nimi: Astronomical Society of the Pacific Conference Series
Vuosikerta: 486
Aloitussivu: 109
Lopetussivu: 114
Sivujen määrä: 6
ISBN: 978-1-58381-856-5
ISSN: 1050-3390
An overview is given of what we know about the frequency of kinematically decoupled cores in dwarf elliptical galaxies. New observations show that kinematically decoupled cores happen just as often in dwarf elliptical as in ordinary early-type galaxies. This has important consequences for the formation of kinematically decoupled cores. Our currently most popular theory for kinematically decoupled cores in dwarf ellipticals is that they were formed in a poor group environment or in isolation, and subsequent fell into the cluster environment where star formation was quenched.
