Physics of the Interstellar Medium « Federica

The course “Physics of the Interstellar Medium” covers the basic physical processes that regulate the state of diffuse gas in, around and between galaxies. Therefore, we will extend our attention also the intergalactic medium, since this is a very vital research area in modern astrophysics. Topics covered include the chemical composition and the phases of the interstellar medium, the equilibrium of gaseous nebulae, the formation of the emission and absorption lines, the properties of the interstellar dust, the molecular gas and the process of star formation, supernova explosions, galactic superwinds. We will also discuss the observational techniques that allow us to investigate the physics of the interstellar and intergalactic media. In particular, we will address the formation of emission and absorption spectral lines (at UV, optical and infrared wavelengths). The goal is to develop the background required to understand current research on the interplay between star formation and cosmic gas. Some lectures will be dedicated to the discussion of recent papers, assigned as complementary readings.

13. The intergalactic medium - first part

Evidence for the IGM The space between field galaxies is also

11-16
20:12

11. Stellar formation in the Orion Nebula

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

11-16
18:44

14. The intergalactic medium - part second

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

11-16
26:00

12. Introduction to the study of the intracluster medium

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

11-16
26:58

10. Ionized systems in the ISM: Warm ionized medium and …

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

11-16
24:20

9. Properties of the interstellar dust

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

11-16
20:20

8. Molecular clouds

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

11-16
28:38

7. Physics of HI clouds

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

11-16
22:40

6. Energy balance in the ISM

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

11-16
21:42

5. Equilibrium configurations the ISM

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

11-16
20:56

4. Matter components of the ISM

Five components of the gaseous ISM In this lecture we will

11-16
17:18

3. A census of systems in the Interstellar Medium, part 2

A census of systems in the ISM We continue our survey

11-16
20:14

2. A census of systems in the Interstellar Medium

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

11-16
27:22

1. Introduction to the study of the physics of the interstellar medium

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

11-16
20:20

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