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          Institute: MPI für Astronomie     Collection: Publikationen_mpia     Display Documents



ID: 709732.0, MPI für Astronomie / Publikationen_mpia
Stellar kinematics and structural properties of Virgo cluster dwarf early-type galaxies from the SMAKCED project. II. The survey and a systematic analysis of kinematic anomalies and asymmetries
Authors:Toloba, E.; Guhathakurta, P.; Peletier, R. F.; Boselli, A.; Lisker, T.; Falcón-Barroso, J.; Simon, J. D.; van de Ven, G.; Paudel, S.; Emsellem, E.; Janz, J.; den Brok, M.; Gorgas, J.; Hensler, G.; Laurikainen, E.; Niemi, S. -. M.; Rys, A.; Salo, H.
Date of Publication (YYYY-MM-DD):2014
Title of Journal:The Astrophysical Journal Supplement Series
Volume:215
Issue / Number:2
Start Page:id. 17 (51 pp)
Audience:Not Specified
Abstract / Description:We present spatially resolved kinematics and global stellar populations and mass-to-light ratios for a sample of 39 dwarf early-type (dE) galaxies in the Virgo cluster studied as part of the SMAKCED stellar absorption-line spectroscopy and imaging survey. This sample is representative of the early-type population in the Virgo cluster in the absolute magnitude range -19.0 < Mr < -16.0 and of all morphological subclasses found in this galaxy population. For each dE, we measure the rotation curve and velocity dispersion profile and fit an analytic function to the rotation curve. We study the significance of the departure of the rotation curve from the best-fit analytic function (poorly fit) and of the difference between the approaching and receding sides of the rotation curve (asymmetry). Our sample includes two dEs with kinematically decoupled cores that have been previously reported. We find that 62 ± 8% (23 out of the 39) of the dEs have a significant anomaly in their rotation curve. Analysis of the images reveals photometric anomalies for most galaxies. However, there is no clear correlation between the significance of the photometric and kinematic anomalies. We measure age-sensitive (Hbeta and HgammaA ) and metallicity sensitive (Fe4668 and Mgb) Lick spectral indices in the LIS-5 Å system. This population of galaxies exhibits a wide range of ages and metallicities; we also find that 4 dEs show clear evidence of emission partially filling in the Balmer absorption lines. Finally, we estimate the total masses and dark matter fractions of the dEs and plot them in the mass-size, the mass-velocity dispersion, and the fundamental plane scaling relations. The dEs seem to be the bridge between massive early-type galaxies and dSphs, and have a median total mass within the Re of log Me = 9.1 ± 0.2 and a median dark matter fraction within the Re of f DM = 46 ± 18%. Any formation model for the dE galaxy class must account for this diversity of kinematic and photometric anomalies and stellar populations.
Free Keywords:galaxies: dwarf; galaxies: elliptical and lenticular; cD; galaxies: clusters: individual: Virgo; galaxies: kinematics and dynamics; galaxies: stellar content; galaxies: photometry
External Publication Status:published
Document Type:Article
Communicated by:N. N.
Affiliations:MPI für Astronomie
Identifiers:ISSN:0067-0049 %R 10.1088/0067-0049/215/2/17
URL:http://cdsads.u-strasbg.fr/abs/2014ApJS..215...17T
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