Physics of the Interstellar Medium « Federica: Recent Episodes

Giovanni Covone

Il Web Learning dell'Università degli Studi di Napoli Federico II

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Evidence for the IGM The space between field galaxies is also

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The ISM systems in Orion The Giant Molecular Cloud in Orion. The

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IGM absorption lines Ionized medium up to z=5 Considering that is

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Introduction: the ICM The space among galaxies is not as empty. Astrophysical

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The diffuse "warm ionized medium" The diffuse "warm ionized medium" (WIM):

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First evidence for dust extinction Trumpler (1930) demonstrated the existence of

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History of observations of dark clouds "Here is truly a hole

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Introduction The dominant component in the ISM is hydrogen. Atomic hydrogen (HI)

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Magnetic fields in the Orion Molecular Cloud Introduction In the last lecture

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Introduction Topic of this lecture: equilibrium configuration in the ISM systems. Thermodynamical

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Five components of the gaseous ISM In this lecture we will

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A census of systems in the ISM We continue our survey

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What is the ISM What is the ISM made of: a

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Preface What is the interstellar medium? The term "interstellar medium" (ISM) refers