Searching for disks around high-mass (proto)stars with ALMA R. Cesaroni, H. Zinnecker, M.T. Beltrán, S. Etoka, D. Galli, C. Hummel, N. Kumar, L. Moscadelli,
Thomas Henning and Dima Semenov Chemistry and Dynamics in Protoplanetary Disks Max-Planck-Institut für Astronomie, Heidelberg Courtesy of David E. Trilling.
The Formation of Stars Chapter 11. Previous chapters have used the basic principles of physics as a way to deduce things about stars and the interstellar.
THE BEAGLE 2 LANDER The British led effort to land on Mars, as part of the European Space Agency's Mars Express Mission, to be launched in June 2003. Beagle2,
Parkinson
Molecular Opacities and Collisional Processes for IR/Sub-mm Brown Dwarf and Extrasolar Planet Modeling Phillip C. Stancil Department of Physics and Astronomy.
Formation of Stars Physics 113 Goderya Chapter(s):11 Learning Outcomes:
Allen et al. (2005) Johnstone et al. (2000). Oph B2 850 m continuum (JCMT) NH 3 (1,1) int. intensity (GBT) NH 3 emission shows excellent (but not perfect)
M. Emprechtinger, D. Lis, P. Schilke, R. Rolffs, R. Monje, The Chess Team.
Chapter 25 Review Questions. 25.1 1a. In this model of the solar system – The sun is in the center of the universe. Heliocentric or Geocentric? 1b. True.
Ch 27 Review Planets & the Solar System. Name the inner planets.
Effective area at 40GHz ~ 10x JVLA? Frequency range: 1 – 50, 70 – 115 GHz? ~18m antennas w. 50% to few km + 40% to 200km + 10% to 3000km?
