Why and when is internally driven AGN feedback energetically favoured?
Version of Record online: 1 MAY 2012
© 2012 The Author Monthly Notices of the Royal Astronomical Society © 2012 RAS
Monthly Notices of the Royal Astronomical Society
Volume 427, Issue 1, pages 2–10, 21 November 2012
How to Cite
Pope, E. C. D. (2012), Why and when is internally driven AGN feedback energetically favoured?. Monthly Notices of the Royal Astronomical Society, 427: 2–10. doi: 10.1111/j.1365-2966.2012.21046.x
- Issue online: 29 OCT 2012
- Version of Record online: 1 MAY 2012
- Manuscript Accepted: 2 APR 2012
- Manuscript Received: 26 MAR 2012
Options for accessing this content:
- If you are a society or association member and require assistance with obtaining online access instructions please contact our Journal Customer Services team.
- Login via other institutional login options http://onlinelibrary.wiley.com/login-options.
Login via OpenAthens
Search for your institution's name below to login via Shibboleth.
Registered Users please login:
- Access your saved publications, articles and searches
- Manage your email alerts, orders and subscriptions
- Change your contact information, including your password
Please register to:
- Save publications, articles and searches
- Get email alerts
- Get all the benefits mentioned below!