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The ATLAS^(3D) project – XXIV. The intrinsic shape distribution of early-type galaxies

Weijmans, Anne-Marie and Alatalo, Katherine (2014) The ATLAS^(3D) project – XXIV. The intrinsic shape distribution of early-type galaxies. Monthly Notices of the Royal Astronomical Society, 444 (1). pp. 3340-3356. ISSN 0035-8711. https://resolver.caltech.edu/CaltechAUTHORS:20141121-103841827

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Abstract

We use the ATLAS^(3D) 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. The so-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 σ_q = 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 σ_q = 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.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://arxiv.org/abs/1408.1099arXivDiscussion Paper
http://mnras.oxfordjournals.org/content/444/4/3340.abstractPublisherArticle
http://dx.doi.org/ 10.1093/mnras/stu1603DOIArticle
ORCID:
AuthorORCID
Alatalo, Katherine0000-0002-4261-2326
Additional Information:© 2014 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society. Accepted 2014 August 5. Received 2014 August 5; in original form 2013 February 9. First published online September 17, 2014. The authors thank Arjen van der Wel for kindly sharing his data, as well as fruitful discussions. The authors also thank the referee for constructive comments. This work was supported by the rolling grants Astrophysics at Oxford PP/E001114/1 and ST/H002456/1 and visitors grants PPA/V/S/2002/00553, PP/E001564/1 and ST/H504862/1 from the UK Research Councils. RLD acknowledges travel and computer grants from Christ Church, Oxford and support from the Royal Society in the form of a Wolfson Merit Award 502011.K502/jd. RLD is also grateful for support from the Australian Astronomical Observatory Distinguished Visitors programme, the ARC Centre of Excellence for All Sky Astrophysics and the University of Sydney during a sabbatical visit. MC acknowledges support from a Royal Society University Research Fellowship. SK acknowledges support from the Royal Society Joint Projects Grant JP0869822. RMMcD is supported by the Gemini Observatory, which is operated by the Association of Universities for Research in Astronomy, Inc., on behalf of the international Gemini partnership of Argentina, Australia, Brazil, Canada, Chile, the United Kingdom and the United States of America. TN and MBois acknowledge support from the DFG Cluster of Excellence ‘Origin and Structure of the Universe’. MS acknowledges support from a STFC Advanced Fellowship ST/F009186/1. PS acknowledges support of a NWO/Veni grant. TAD has received funding from the European Community’s Seventh Framework Programme (/FP7/2007-2013/) under grant agreement No 229517. MBois has received, during this research, funding from the European Research Council under the Advanced Grant Program Num 267399-Momentum. LMY acknowledges support from NSF AST-1109803. The authors acknowledge financial support from ESO. This paper is based on observations obtained at the William Herschel Telescope and the Isaac Newton Telescope, operated by the Isaac Newton Group in the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofísica de Canarias. Funding for the SDSS and SDSS-II was provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, the US Department of Energy, the National Aeronautics and Space Administration, the Japanese Monbukagakusho, the Max Planck Society and the Higher Education Funding Council for England. The SDSS was managed by the Astrophysical Research Consortium for the Participating Institutions. This publication makes use of data products from the Wide-field Infrared Survey Explorer, which is a joint project of the University of California, Los Angeles, and the Jet Propulsion Laboratory/California Institute of Technology, funded by the National Aeronautics and Space Administration.
Group:Infrared Processing and Analysis Center (IPAC)
Funders:
Funding AgencyGrant Number
Particle Physics and Astronomy Research Council (PPARC)PP/E001114/1
Science and Technology Facilities Council (STFC)ST/H002456/1
Particle Physics and Astronomy Research Council (PPARC)PPA/V/S/2002/00553
Particle Physics and Astronomy Research Council (PPARC)PP/E001564/1
Science and Technology Facilities Council (STFC)ST/H504862/1
Royal Society502011.K502/jd
Australian Astronomical Observatory (AAO)UNSPECIFIED
Australian Research CouncilUNSPECIFIED
Royal SocietyJP0869822
Gemini ObservatoryUNSPECIFIED
Deutsche Forschungsgemeinschaft (DFG)UNSPECIFIED
Science and Technology Facilities Council (STFC)ST/F009186/1
Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO)UNSPECIFIED
European Research Council (ERC)229517
European Research Council (ERC)267399-Momentum
NSFAST-1109803
European Southern Observatory (ESO)UNSPECIFIED
Alfred P. Sloan FoundationUNSPECIFIED
Department of Energy (DOE)UNSPECIFIED
NASAUNSPECIFIED
Japanese MonbukagakushoUNSPECIFIED
Max Planck SocietyUNSPECIFIED
Higher Education Funding Council for EnglandUNSPECIFIED
NASA/JPL/CaltechUNSPECIFIED
Subject Keywords:galaxies: elliptical and lenticular, cD galaxies: structure
Issue or Number:1
Record Number:CaltechAUTHORS:20141121-103841827
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20141121-103841827
Official Citation:Anne-Marie Weijmans, P. T. de Zeeuw, Eric Emsellem, Davor Krajnović, Pierre-Yves Lablanche, Katherine Alatalo, Leo Blitz, Maxime Bois, Frédéric Bournaud, Martin Bureau, Michele Cappellari, Alison F. Crocker, Roger L. Davies, Timothy A. Davis, Pierre-Alain Duc, Sadegh Khochfar, Harald Kuntschner, Richard M. McDermid, Raffaella Morganti, Thorsten Naab, Tom Oosterloo, Marc Sarzi, Nicholas Scott, Paolo Serra, Gijs Verdoes Kleijn, and Lisa M. Young The ATLAS 3D project – XXIV. The intrinsic shape distribution of early-type galaxies MNRAS (November 11, 2014) Vol. 444 3340-3356 doi:10.1093/mnras/stu1603 First published online September 17, 2014
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:52042
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:21 Nov 2014 20:43
Last Modified:03 Oct 2019 07:38

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