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The ATLAS3D project - XXIV. The intrinsic shape distribution of early-type galaxies

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1408.1099.pdf (1.297Mb)
Date
11/11/2014
Author
Weijmans, Anne-Marie
de Zeeuw, P. T.
Emsellem, Eric
Krajnovic, Davor
Lablanche, Pierre-Yves
Alatalo, Katherine
Blitz, Leo
Bois, Maxime
Bournaud, Frederic
Bureau, Martin
Cappellari, Michele
Crocker, Alison
Davies, Roger
Davis, Timothy
Duc, Pierre-Alain
Khochfar, Sadegh
Kuntschner, Harald
McDermid, Richard
Morganti, Raffaella
Naab, Thorsten
Oosterloo, Tom
Sarzi, Marc
Scott, Nicholas
Serra, Paolo
Verdoes Kleijn, Gijs
Young, Lisa
Keywords
Galaxies: elliptical and lenticular, cD
Galaxies: structure
QB Astronomy
QC Physics
BDC
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Abstract
We use the ATLAS3D sample to perform a study of the intrinsic shapes of early-type galaxies, taking advantage of the available combined photometric and kinematic data. Based on our ellipticity measurements from the Sloan Digital Sky Survey Data Release 7, and additional imaging from the Isaac Newton Telescope, we first invert the shape distribution of fast and slow rotators under the assumption of axisymmetry. Theso-obtained intrinsic shape distribution for the fast rotators can be described with a Gaussian with a mean flattening of q=0.25 and standard deviation σq = 0.14, and an additional tail towards rounder shapes.The slow rotators are much rounder, and are well described with a Gaussian with mean q = 0.63 and σq =0.09. We then checked that our results were consistent when applying a different and independent method to obtain intrinsic shape distributions, by fitting the observed ellipticity distributions directly using Gaussian parametrizations for the intrinsic axis ratios. Although both fast and slow rotators are identified as early-type galaxies in morphological studies, and in many previous shape studies are therefore grouped together, their shape distributions are significantly different, hinting at different formation scenarios. The intrinsic shape distribution of the fast rotators shows similarities with the spiral galaxy population. Including the observed kinematic misalignment in our intrinsic shape study shows that the fast rotators are predominantly axisymmetric, with only very little room for triaxiality. For the slow rotators though there are very strong indications that they are (mildly) triaxial.
Citation
Weijmans , A-M , de Zeeuw , P T , Emsellem , E , Krajnovic , D , Lablanche , P-Y , Alatalo , K , Blitz , L , Bois , M , Bournaud , F , Bureau , M , Cappellari , M , Crocker , A , Davies , R , Davis , T , Duc , P-A , Khochfar , S , Kuntschner , H , McDermid , R , Morganti , R , Naab , T , Oosterloo , T , Sarzi , M , Scott , N , Serra , P , Verdoes Kleijn , G & Young , L 2014 , ' The ATLAS 3D project - XXIV. The intrinsic shape distribution of early-type galaxies ' , Monthly Notices of the Royal Astronomical Society , vol. 444 , no. 4 , pp. 3340-3356 . https://doi.org/10.1093/mnras/stu1603
Publication
Monthly Notices of the Royal Astronomical Society
Status
Peer reviewed
DOI
https://doi.org/10.1093/mnras/stu1603
ISSN
0035-8711
Type
Journal article
Rights
© 2014. The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society
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  • University of St Andrews Research
URL
http://adsabs.harvard.edu/abs/2014arXiv1408.1099W
URI
http://hdl.handle.net/10023/5450

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