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The top documents tagged [diffuse gas]

Galaxy feedback in 3D Roberto Maiolino. Feedback is the key: - reducing SF efficiency (gas heating+turbulence) - removing baryons Discrepancy between
Galaxy feedback in 3D Roberto Maiolino. Feedback is the key: - reducing SF efficiency (gas heating+turbulence) - removing baryons Discrepancy between
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Potential Habitable Exoplanets: Interstellar Space Travel As Mankind's Salvation
Potential Habitable Exoplanets: Interstellar Space Travel As Mankind's Salvation
453 views
Chemistry universe chandra
Chemistry universe chandra
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Cosmic Microwave Background, Foregrounds and Component Separation What are foregrounds and how to deal with them in CMB data analysis Carlo Baccigalupi,
Cosmic Microwave Background, Foregrounds and Component Separation What are foregrounds and how to deal with them in CMB data analysis Carlo Baccigalupi,
215 views
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)
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)
215 views
Intrinsic Absorption in Quasars: BALs & NALs Jonathan Trump February 11, 2007
Intrinsic Absorption in Quasars: BALs & NALs Jonathan Trump February 11, 2007
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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
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
216 views
Harvey LisztLondon, January 2006 Harvey Liszt NRAO, CHARLOTTESVILLE
Harvey LisztLondon, January 2006 Harvey Liszt NRAO, CHARLOTTESVILLE
220 views
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
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
214 views
The Galactic center region Concentrated stars and interstellar matter High energy density (gravity, MHD, kinetic) Strong magnetic field :B ~ mG High external
The Galactic center region Concentrated stars and interstellar matter High energy density (gravity, MHD, kinetic) Strong magnetic field :B ~ mG High external
218 views
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
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
228 views
The Interaction of Light and Matter Spectral Lines Photons Rutherford-Bohr Model of the Atom Quantum Mechanics and Wave-Particle Duality
The Interaction of Light and Matter Spectral Lines Photons Rutherford-Bohr Model of the Atom Quantum Mechanics and Wave-Particle Duality
218 views