Physics of the Interstellar Medium « Federica

Physics of the Interstellar Medium « Federica episodes:

• November 16, 201113. The intergalactic medium - first part

  Evidence for the IGM The space between field galaxies is also

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• November 16, 201111. Stellar formation in the Orion Nebula

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

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• November 16, 201114. The intergalactic medium - part second

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

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• November 16, 201112. Introduction to the study of the intracluster medium

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

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• November 16, 201110. Ionized systems in the ISM: Warm ionized medium and …

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

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• November 16, 20119. Properties of the interstellar dust

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

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• November 16, 20118. Molecular clouds

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

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• November 16, 20117. Physics of HI clouds

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

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• November 16, 20116. Energy balance in the ISM

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

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• November 16, 20115. Equilibrium configurations the ISM

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

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