The Quasar Absorption Line - Galaxy Evolution Group

Studying the Evolution of Galaxies

We are a collaborative group of the Astronomy Departments at New Mexico State University, Penn State, and Swinburne University of Techonology (Australia). We are engaged in research using the technique of quasar absorption lines to study the kinematic, ionization, and chemical conditions of gas associated with intermediate and high redshift galaxies and simulations to understand the general evolution of galaxies. Our goals are to contribute to the growing body of knowledge of the role of gas in galaxy formation and evolution.


| Our Science | Talk Videos | HST-GO-13398 | MAGIICAT |

FACULTY
Jane
Charlton

(Penn State)
Glenn
Kacprzak

(Swinburne)
Michael
Murphy

(Swinburne)
POST DOC/
COLLABORATORS
Daniel
Ceverino


(Madrid)
Nikki
Nielsen


(Swinburne)

Sowgat
Muzahid


(Penn State)

NMSU GRAD STUDENTS

This page created and maintained by Chris Churchill; last update: Jan 2016