Chelen Johnson
Investigtating Moving-group Photometry and Understanding Lightcurve Structures (IMPULS) will be studying rotation rates of stars in the young nearby Beta Pic Moving Group.
I wanted to share this with you about one of the students I had on our team that explored star formation in Lynds dark nebulae (LDNs) [in 2008]. [He has since become involved with a big Air Force program at Michigan Tech in 2012.] [He] has often thanked me for getting him involved in NITARP research, having used that experience, in part, to get access to programs such as MTU's Aerospace Enterprise.
NITARP has been the best experience I have ever had for my personal and professional development as an astronomy educator.
Finally much of the [AAS 2009] invited talk by Eugene Churazov on Galaxy Clusters and Black Holes I found to be understandable because he used many equations from ideal gas laws that are familiar to high school teachers and their students. In talking with Dr. Churazov after his talk, he re-emphasized how far one could go on this topic with these familiar and seemingly simple equations.
