Skip to main content Accessibility help
×
Home
Hostname: page-component-55597f9d44-2qt69 Total loading time: 0.254 Render date: 2022-08-18T05:58:15.070Z Has data issue: true Feature Flags: { "shouldUseShareProductTool": true, "shouldUseHypothesis": true, "isUnsiloEnabled": true, "useRatesEcommerce": false, "useNewApi": true } hasContentIssue true

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
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
Rights & Permissions[Opens in a new window]

Extract

HTML view is not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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
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
You have Access

Save article to Kindle

To save this article to your Kindle, first ensure coreplatform@cambridge.org is added to your Approved Personal Document E-mail List under your Personal Document Settings on the Manage Your Content and Devices page of your Amazon account. Then enter the ‘name’ part of your Kindle email address below. Find out more about saving to your Kindle.

Note you can select to save to either the @free.kindle.com or @kindle.com variations. ‘@free.kindle.com’ emails are free but can only be saved to your device when it is connected to wi-fi. ‘@kindle.com’ emails can be delivered even when you are not connected to wi-fi, but note that service fees apply.

Find out more about the Kindle Personal Document Service.

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

Save article to Dropbox

To save this article to your Dropbox account, please select one or more formats and confirm that you agree to abide by our usage policies. If this is the first time you used this feature, you will be asked to authorise Cambridge Core to connect with your Dropbox account. Find out more about saving content to Dropbox.

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

Save article to Google Drive

To save this article to your Google Drive account, please select one or more formats and confirm that you agree to abide by our usage policies. If this is the first time you used this feature, you will be asked to authorise Cambridge Core to connect with your Google Drive account. Find out more about saving content to Google Drive.

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

Reply to: Submit a response

Please enter your response.

Your details

Please enter a valid email address.

Conflicting interests

Do you have any conflicting interests? *