Skip to main content Accessibility help
×
Home
Hostname: page-component-684bc48f8b-v5sh4 Total loading time: 0.327 Render date: 2021-04-13T16:37:32.751Z Has data issue: true Feature Flags: { "shouldUseShareProductTool": true, "shouldUseHypothesis": true, "isUnsiloEnabled": true, "metricsAbstractViews": false, "figures": false, "newCiteModal": false, "newCitedByModal": true }

Evolution of disk galaxies in MOdified Gravity (MOG)

Published online by Cambridge University Press:  14 May 2020

Neda Ghafourian
Affiliation:
Department of Physics, Faculty of Science, Ferdowsi University of Mashhad, P.O. Box 1436, Mashhad, Iran emails: n.ghafourian@mail.um.ac.ir, mroshan@um.ac.ir
Mahmood Roshan
Affiliation:
Department of Physics, Faculty of Science, Ferdowsi University of Mashhad, P.O. Box 1436, Mashhad, Iran emails: n.ghafourian@mail.um.ac.ir, mroshan@um.ac.ir
Corresponding

Abstract

Evolution and the formation of bars in the galactic disks is studied in the context of Modified Gravity (MOG) by using N-body simulations. It is found that changing the value of free parameters of the model can effectively alter the strength of the bar and disk’s stability.

Type
Contributed Papers
Copyright
© International Astronomical Union 2020

Access options

Get access to the full version of this content by using one of the access options below.

References

Moffat, J. W. 2006, JCAP, 0603, 00410.1088/1475-7516/2006/03/004CrossRefGoogle Scholar
Moffat, J. W. & Rahvar, S 2013, MNRAS, 436, 1439145110.1093/mnras/stt1670CrossRefGoogle Scholar
Haghi, H. & Amiri, V. 2016, MNRAS, 463, 2, 194410.1093/mnras/stw2140CrossRefGoogle Scholar
Green, M. A. & Moffat, J. W. 2019, PDU, 25, 323Google Scholar
Sellwood, J. A. 2016, ApJ, 819, 9210.3847/0004-637X/819/2/92CrossRefGoogle Scholar
Ghafourian, N. & Roshan, M. 2017, MNRAS, 468, 4450CrossRefGoogle Scholar
Roshan, M. 2018, ApJ, 854, 38CrossRefGoogle Scholar
Sellwood, J. A. 2014, arxiv eprint, 1406.6606Google Scholar

Full text views

Full text views reflects PDF downloads, PDFs sent to Google Drive, Dropbox and Kindle and HTML full text views.

Total number of HTML views: 0
Total number of PDF views: 18 *
View data table for this chart

* Views captured on Cambridge Core between 14th May 2020 - 13th April 2021. This data will be updated every 24 hours.

Send article to Kindle

To send this article to your Kindle, first ensure no-reply@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 sending to your Kindle. Find out more about sending to your Kindle.

Note you can select to send to either the @free.kindle.com or @kindle.com variations. ‘@free.kindle.com’ emails are free but can only be sent 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.

Evolution of disk galaxies in MOdified Gravity (MOG)
Available formats
×

Send article to Dropbox

To send 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 use this feature, you will be asked to authorise Cambridge Core to connect with your <service> account. Find out more about sending content to Dropbox.

Evolution of disk galaxies in MOdified Gravity (MOG)
Available formats
×

Send article to Google Drive

To send 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 use this feature, you will be asked to authorise Cambridge Core to connect with your <service> account. Find out more about sending content to Google Drive.

Evolution of disk galaxies in MOdified Gravity (MOG)
Available formats
×
×

Reply to: Submit a response


Your details


Conflicting interests

Do you have any conflicting interests? *