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Variations in the Fundamental Plane of massive galaxies with stellar population, morphology and local density

Published online by Cambridge University Press:  17 July 2013

Christina Magoulas ,
Christopher Springob ,
Rob Proctor ,
Matthew Colless ,
D. Heath Jones ,
Chiaki Kobayashi ,
Lachlan Campbell ,
John Lucey  and
Jeremy Mould
Christina Magoulas
Affiliation:
AAO U. Melbourne, email: c.magoulas@pgrad.unimelb.edu.au
Christopher Springob
Affiliation:
AAO
Rob Proctor
Affiliation:
U. São Paulo
Matthew Colless
Affiliation:
AAO
D. Heath Jones
Affiliation:
Monash University
Chiaki Kobayashi
Affiliation:
ANU
Lachlan Campbell
Affiliation:
WKU
John Lucey
Affiliation:
Durham University
Jeremy Mould
Affiliation:
Swinburne University
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We have measured Fundamental Plane (FP) parameters in the 2MASS J, H and K passbands for 10,000 ellipticals, lenticulars and early-type spiral bulges in the 6dF Galaxy Survey (6dFGS) – a spectroscopic survey of the southern sky with |b| > 10° (Jones et al. 2009). 6dFGS provides a large near-infrared-selected sample of galaxies for accurately determining the NIR FP and investigating the trends in the FP with stellar population, morphology and environment.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S295: The intriguing life of massive galaxies , August 2012 , pp. 233
Copyright
Copyright © International Astronomical Union 2013 

References

Jones, D. H., et al. 2009, MNRAS, 399, 683CrossRefGoogle Scholar
Magoulas, C., et al. 2009, MNRAS, 427, 245CrossRefGoogle Scholar
Springob, C. M., et al. 2012, MNRAS, 420, 2773CrossRefGoogle Scholar