'Dense clouds' diaporamas de présentation

Science (1999) Vol. 283 p 1135-1138

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The Origin of Our Solar System Part 1

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Chapter 21

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Nick Indriolo Johns Hopkins University (University of Illinois at Urbana-Champaign)

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CONDITIONS IN DENSE INTERSTELLAR CLOUDS

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Dissociative Recombination of Cold H 3 + and its Interstellar Implications

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H 3 + : A new probe of the Galactic center

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Exploring the Central Molecular Zone of the Galaxy using H 3 + and CO July 11,1997- present

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Nick Indriolo , 1 Ben McCall, 1 Tom Geballe, 2 & Takeshi Oka 3

Investigating the Cosmic-Ray Ionization Rate in the Galactic Interstellar Medium through Observations of H 3 +. Nick Indriolo , 1 Ben McCall, 1 Tom Geballe, 2 & Takeshi Oka 3 1 University of Illinois at Urbana-Champaign; 2 Gemini Observatory; 3 University of Chicago. Introduction.

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Constraining the Flux of Low-Energy Cosmic Rays Accelerated by the Supernova Remnant IC 443

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11 year cycle Sun spots Solar Flares

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The Traveling Exhibit

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AGN: Quasars

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H 3 + Toward and Within the Galactic Center

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Theories on how the dinosaurs became extinct

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