Main content

Detecting Inflowing Gas in Mg II and Fe II at Intermediate Redshift

  0
Contributors:

Date created: | Last Updated:

: DOI | ARK

Creating DOI. Please wait...

Create DOI

Category: Project

Wiki

I will discuss the results of two Keck studies that trace low-ionization gas flows in and out of intermediate redshift galaxies. Using LRIS spectroscopy of 200 galaxies at 0.4 < z < 1.4, we find that detections of gas inflows as traced by Mg II and Fe II are not as common as gas outflows, when viewed “down the barrel” towards each galaxy. The inflowing gas typically has velocities of 100-200 km…

Files

Files can now be accessed and managed under the Files tab.

Citation

Tags

NRAO2015talk

Recent Activity

Unable to retrieve logs at this time. Please refresh the page or contact support@osf.io if the problem persists.

OSF does not support the use of Internet Explorer. For optimal performance, please switch to another browser.
Accept
This website relies on cookies to help provide a better user experience. By clicking Accept or continuing to use the site, you agree. For more information, see our Privacy Policy and information on cookie use.
Accept
×

Start managing your projects on the OSF today.

Free and easy to use, the Open Science Framework supports the entire research lifecycle: planning, execution, reporting, archiving, and discovery.

Copyright © 2011-2025 Center for Open Science | Terms of Use | Privacy Policy | Status | API
TOP Guidelines | Reproducibility Project: Psychology | Reproducibility Project: Cancer Biology