Dust in Dwarf Galaxies Adam Leroy N ATIONAL R ADIO A STRONOMY O BSERVATORY HERITAGE (Meixner et al.)
Expanded Polytetrafluoroethylene Membrane Surface Modification Using Acetylene-nitrogen Plasma Treatment
Clusters of galaxies The ICM, mass measurements and statistical measures of clustering.
On the Star Formation Rates in GMCs with Marco Lombardi, Joao Alves, Jan Forbrich, Gus Munch Kevin Covey & Carlos Roman.
ESO Galaxy Formation: The Radio Decade (Dense Gas History of the Universe) Chris Carilli (NRAO) Santa Fe, March 2011 Power of radio astronomy: dust, cool.
1 National Radio Astronomy Observatory – Town Hall AAS 211 th Meeting – Austin, Texas Science Synergies with NRAO Telescopes Chris Carill NRAO.
SMA [CII] 158um 334GHz, 20hrs BRI1202-0725 z=4.7 Quasar-SMG pair Both HyLIRG Both detected in CO Iono ea 2007 Omont ea. 1996 + + 4”4” HST 814 Hu ea 96.
ESO
Current and Future Science with NRAO Instruments
Science Synergies with NRAO Telescopes
Eruptive Mass Loss in Massive Stars Nathan Smith - University of Arizona
80x Bandwidth (8 GHz, full stokes), with 4000 channels Full frequency coverage (1 to 50 GHz)