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El. knyga: Interstellar Medium, Expanding Nebulae and Triggered Star Formation: Theory and Simulations

  • Formatas: PDF+DRM
  • Serija: SpringerBriefs in Astronomy
  • Išleidimo metai: 24-Nov-2015
  • Leidėjas: Springer International Publishing AG
  • Kalba: eng
  • ISBN-13: 9783319261423
Kitos knygos pagal šią temą:
  • Formatas: PDF+DRM
  • Serija: SpringerBriefs in Astronomy
  • Išleidimo metai: 24-Nov-2015
  • Leidėjas: Springer International Publishing AG
  • Kalba: eng
  • ISBN-13: 9783319261423
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This brief brings together the theoretical aspects of star formation and ionized regions with the most up-to-date simulations and observations. Beginning with the basic theory of star formation, the physics of expanding HII regions is reviewed in detail and a discussion on how a massive star can give birth to tens or hundreds of other stars follows. The theoretical description of star formation is shown in simplified and state-of-the-art numerical simulations, describing in a more clear way how feedback from massive stars can trigger star and planet formation. This is also combined with spectacular images of nebulae taken by talented amateur astronomers. The latter is very likely to stimulate the reader to observe the structure of nebulae from a different point of view, and better understand the associated star formation therein.
1 The Interstellar Medium
1(16)
1.1 Overview
1(4)
1.2 The Dusty ISM
5(3)
1.3 Interstellar Radiation Field
8(1)
1.4 Photodissociation Regions
8(3)
1.5 Cosmic Rays
11(2)
1.6 Detection of H2
13(1)
1.7 Life Cycle of the Stars and the ISM
14(3)
References
15(2)
2 Nebulae
17(18)
2.1 Ionization and Recombination of Hydrogen
17(2)
2.2 Categories of Nebulae
19(5)
2.2.1 Diffuse (Emission) Nebulae
20(1)
2.2.2 Planetary Nebulae
21(1)
2.2.3 Supernova Remnants
22(1)
2.2.4 Reflection and Dark Nebulae
23(1)
2.3 Photoionization Equilibrium
24(3)
2.4 Heating and Cooling Mechanisms
27(1)
2.5 R-Type Expansion
28(1)
2.6 D-Type Expansion
29(6)
2.6.1 Further Discussion
32(2)
References
34(1)
3 Triggered Star Formation
35(16)
3.1 Overview
35(3)
3.2 Gravitational Collapse
38(2)
3.3 Instabilities During the D-Type Phase
40(4)
3.3.1 Vishniac Instability
40(2)
3.3.2 Rayleigh-Taylor Instability
42(2)
3.4 Collect and Collapse
44(2)
3.5 Radiation-Driven Implosion
46(1)
3.6 The Formation of Our Solar System
47(4)
References
49(2)
4 Numerical Simulations
51(18)
4.1 Introduction
51(2)
4.2 Methods Followed in Numerical Simulations
53(4)
4.2.1 Grid-Based Methods
54(1)
4.2.2 Smoothed Particle Hydrodynamics Methods
55(2)
4.2.3 Hybrid Methods
57(1)
4.3 Simulations
57(7)
4.3.1 Spherically Symmetric Expansion
59(1)
4.3.2 Off-Center Expansion
59(3)
4.3.3 Radiation Driven Implosion
62(1)
4.3.4 Fractal Clouds
62(2)
4.4 Synthetic Observations
64(5)
References
66(3)
5 Summary
69
Dr. Thomas G. Bisbas is a researcher at the Max-Planck-Institute in Garching (Germany) and at the University of Florida, Gainesville (USA). He received his Ph.D. in Astrophysics from Cardiff University (UK) and his Degree in Physics from the Aristotle University of Thessaloniki (Greece). He has been a postdoctoral researcher at the Academy of Sciences of the Czech Republic, at the University College London (UK) and a visiting researcher at the Harvard-Smithsonian Centre for Astrophysics (USA). His main areas of study include Computational Astrophysics and Astrochemistry of star formation, the interstellar medium and nebulae. He has published several peer-reviewed articles and has given oral presentations in international conferences as well as outreach talks for amateurs astronomers.