The top documents tagged [dense cores]

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,
Documents 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,

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Thomas Henning and Dima Semenov Chemistry and Dynamics in Protoplanetary Disks Max-Planck-Institut für Astronomie, Heidelberg Courtesy of David E. Trilling
Documents Thomas Henning and Dima Semenov Chemistry and Dynamics in Protoplanetary Disks Max-Planck-Institut für Astronomie, Heidelberg Courtesy of David E. Trilling

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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
Documents 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

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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,
Documents 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,

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Parkinson
Documents Parkinson

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Molecular Opacities and Collisional Processes for IR/Sub-mm Brown Dwarf and Extrasolar Planet Modeling Phillip C. Stancil Department of Physics and Astronomy
Documents Molecular Opacities and Collisional Processes for IR/Sub-mm Brown Dwarf and Extrasolar Planet Modeling Phillip C. Stancil Department of Physics and Astronomy

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Formation of Stars Physics 113 Goderya Chapter(s):11 Learning Outcomes:
Documents Formation of Stars Physics 113 Goderya Chapter(s):11 Learning Outcomes:

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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)
Documents 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)

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M. Emprechtinger, D. Lis, P. Schilke, R. Rolffs, R. Monje, The Chess Team
Documents M. Emprechtinger, D. Lis, P. Schilke, R. Rolffs, R. Monje, The Chess Team

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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
Documents 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

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Ch 27 Review Planets & the Solar System. Name the inner planets
Documents Ch 27 Review Planets & the Solar System. Name the inner planets

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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?
Documents 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?

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