Galaxy feedback in 3D Roberto Maiolino. Feedback is the key: - reducing SF efficiency (gas heating+turbulence) - removing baryons Discrepancy between.
Potential Habitable Exoplanets: Interstellar Space Travel As Mankind's Salvation
Chemistry universe chandra
Cosmic Microwave Background, Foregrounds and Component Separation What are foregrounds and how to deal with them in CMB data analysis Carlo Baccigalupi,
The [NII] Line Ratio The ISO 122 m [NII] to SPIFI 205 m line ratio yields the density of the low ionization gas (Figure 5, blue line and circle)
Intrinsic Absorption in Quasars: BALs & NALs Jonathan Trump February 11, 2007.
Hot and diffuse gas near the Galactic center probed by metastable H 3 + Thomas R. Geballe Gemini Observatory Miwa Goto Max-Planck-Institut für Astronomie.
Harvey LisztLondon, January 2006 Harvey Liszt NRAO, CHARLOTTESVILLE.
Warm and Diffuse Gas and High Ionizzation Rate Near the Galactic Center from 140 pc West to 85 pc East of Sgr A* 66th OSU International Symposium, June.
The Galactic center region Concentrated stars and interstellar matter High energy density (gravity, MHD, kinetic) Strong magnetic field :B ~ mG High external.
CHORDATA. Characteristics of ALL Chordates An animal that has, for at least some stage of its life, –A dorsal, hollow nerve cord –A notochord –Pharyngeal.
The Interaction of Light and Matter Spectral Lines Photons Rutherford-Bohr Model of the Atom Quantum Mechanics and Wave-Particle Duality.