Astrophysics Seminar meets in room 358 VAN on Tuesdays from 11:30 am - 12:30 pm.
The format is either Astrophysics Journal club or a research presentation. Journal club papers for the current week are listed at VoxCharta (select University of Iowa). Everyone is encouraged to briefly review the selected papers before seminar. Moderators are expected to provide cookies.
|Jan 24||Dr. Fabian Kislat, Washington University,||The Compton Electron Tracking MeV Astronomy Telescope|
|Jan 31||Dr. Brian Fleming, LASP, University of Colorado,||Technologies to Enable the Next-Generations of Far-UV Sensitive Space Missions|
|Feb 7||Dr. Casey DeRoo, Harvard-Smithsonian Center for Astrophysics||Beyond Chandra and XMM-Newton: Adjustable X-ray Optics for the Lynx Mission|
|Feb 14||Dr. Pascal Saint-Hilaire, UC Berkeley,||The Gamma-Ray Imager/Spectrometer for Solar Flares (GRIPS) and the CUbesat Radio Interferometry Experiment (CURIE): New Instruments for New Frontiers in (solar) Physics|
|Feb 21||Dr. Amy Keesee, Dept. Physics & Astronomy, West Virginia University||Novel Techniques for Measuring Particles in Space|
|Mar 2||Dr. Mark Pulupa), Space Sciences Laboratory, UC Berkeley||Precision Measurements of Solar Wind Electrons Using Plasma and Wave Observations|
|Mar 7||Dr. David M. Miles, University of Alberta||Dense, Multipoint Magnetic Measurements: Enabling Novel Studies of Magnetosphere-Ionosphere Coupling|
|Mar 9||Dr. Allison N. Jaynes, ), LASP, University of Colorado||The Crucial Role of Substorms and Whistler-Mode Chorus Waves in the Rebuilding of Earth's Radiation Belts|
|Mar 28||Prof. Cornelia Lang||The ngVLA (next generation) VLA|
|Apr 7 (Friday)||Prof. Larry Rudnick, Univ. of Minnesota||TBA (tentative)|
|Apr 11||Prof. Jack Scudder||Does Quasi-Neutrality Play a Signifiance Role in Astrophysical Plasmas?|
|Apr 18||Ms. Allison Costa, UI||TBA|
|Apr 25||Dr. Anna Zajczyk,University of Iowa||TBA|
|May 2||Prof. Robert Mutel||Pulsed radio emission from Ultra-cool Dwarfs: Implications for Exoplanets|
A Deep Chandra View of M51 (K. D. Kuntz, Johns Hopkins University)
Chandra has made deep studies of four nearby galaxies; M101, M33, M83, and, most recently, M51. In each case the study is relatively uniform out to the D25 radius. Given the failing soft response, it is unlikely that comparable studies of other galaxies will be made with Chandra. I will review the recent point-source population study of M51 where I argue that the concept of universal luminosity functions needs to be reconsidered. I will then use our data from M101, M83 and M51 to address what I think we are beginning to learn about the diffuse X-ray emission from normal late-type spiral galaxies.