Magnetic Fields and Star Formation: Theory Versus Observations
Magnetic Fields play a key role in the physics of star formation on all scales: from the formation of the large complexes of molecular clouds to the formation of solar-like planetary systems. The plasma physics involved is non-linear and very complex, which requires the development of large numerica...
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| Format: | Elektronisch E-Book |
| Sprache: | English |
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Dordrecht
Springer Netherlands
2004
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| Ausgabe: | 1st ed. 2004 |
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| Online-Zugang: | Volltext |
| Zusammenfassung: | Magnetic Fields play a key role in the physics of star formation on all scales: from the formation of the large complexes of molecular clouds to the formation of solar-like planetary systems. The plasma physics involved is non-linear and very complex, which requires the development of large numerical codes. An additional difficulty is that the detection and study of magnetic fields is not easy from an observational point of view, and therefore theoretical models cannot easily be constrained. In the week from April 21st to 25th in 2003, a meeting was held on the Campus of the Universidad Complutense de Madrid (Spain) to join theoretical and observational efforts to address these issues. The objective was to define a set of relevant problems for the physics of star formation that can be properly addressed with the current or near-future instruments. This book summarizes the results of this intensive week of work. The book is written in a comprehensive manner and reviews our current knowledge of the subject. It also represents an updated account of the ideas and thoughts of the scientists working in the field of Star Formation. The contributions are presented in six chapters which correspond to the six fundamental issues (sessions) on which the discussion was focused during the workshop: the physics of turbulence in the Interstellar Medium (ISM), the formation of structure in the ISM, the formation of stars within dense cores of molecular gas, the physics of accretion disks, the physics of outflows and their interaction with the ISM, and the interaction between the stellar magnetosphere and accretion disk. Each chapter starts with a comprehensive summary written by one of the editors, which includes input from the contributions as well as the editor's own thoughts on the subject. For all these reasons the book is well-suited as a primer to introduce graduate students in the richness of this field of research |
| Beschreibung: | 1 Online-Ressource (V, 516 p) |
| ISBN: | 9789401704915 |
| DOI: | 10.1007/978-94-017-0491-5 |
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| 520 | |a Magnetic Fields play a key role in the physics of star formation on all scales: from the formation of the large complexes of molecular clouds to the formation of solar-like planetary systems. The plasma physics involved is non-linear and very complex, which requires the development of large numerical codes. An additional difficulty is that the detection and study of magnetic fields is not easy from an observational point of view, and therefore theoretical models cannot easily be constrained. In the week from April 21st to 25th in 2003, a meeting was held on the Campus of the Universidad Complutense de Madrid (Spain) to join theoretical and observational efforts to address these issues. The objective was to define a set of relevant problems for the physics of star formation that can be properly addressed with the current or near-future instruments. This book summarizes the results of this intensive week of work. The book is written in a comprehensive manner and reviews our current knowledge of the subject. It also represents an updated account of the ideas and thoughts of the scientists working in the field of Star Formation. The contributions are presented in six chapters which correspond to the six fundamental issues (sessions) on which the discussion was focused during the workshop: the physics of turbulence in the Interstellar Medium (ISM), the formation of structure in the ISM, the formation of stars within dense cores of molecular gas, the physics of accretion disks, the physics of outflows and their interaction with the ISM, and the interaction between the stellar magnetosphere and accretion disk. Each chapter starts with a comprehensive summary written by one of the editors, which includes input from the contributions as well as the editor's own thoughts on the subject. For all these reasons the book is well-suited as a primer to introduce graduate students in the richness of this field of research | ||
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| author2 | Gómez de Castro, Ana I. Heyer, Mark Vázquez-Semadeni, Enrique Rebolo, Rafael |
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| edition | 1st ed. 2004 |
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| spelling | Magnetic Fields and Star Formation Theory Versus Observations edited by Ana I. Gómez de Castro, Mark Heyer, Enrique Vázquez-Semadeni, Rafael Rebolo, Michel Tagger, Ralph E. Pudritz 1st ed. 2004 Dordrecht Springer Netherlands 2004 1 Online-Ressource (V, 516 p) txt rdacontent c rdamedia cr rdacarrier Magnetic Fields play a key role in the physics of star formation on all scales: from the formation of the large complexes of molecular clouds to the formation of solar-like planetary systems. The plasma physics involved is non-linear and very complex, which requires the development of large numerical codes. An additional difficulty is that the detection and study of magnetic fields is not easy from an observational point of view, and therefore theoretical models cannot easily be constrained. In the week from April 21st to 25th in 2003, a meeting was held on the Campus of the Universidad Complutense de Madrid (Spain) to join theoretical and observational efforts to address these issues. The objective was to define a set of relevant problems for the physics of star formation that can be properly addressed with the current or near-future instruments. This book summarizes the results of this intensive week of work. The book is written in a comprehensive manner and reviews our current knowledge of the subject. It also represents an updated account of the ideas and thoughts of the scientists working in the field of Star Formation. The contributions are presented in six chapters which correspond to the six fundamental issues (sessions) on which the discussion was focused during the workshop: the physics of turbulence in the Interstellar Medium (ISM), the formation of structure in the ISM, the formation of stars within dense cores of molecular gas, the physics of accretion disks, the physics of outflows and their interaction with the ISM, and the interaction between the stellar magnetosphere and accretion disk. Each chapter starts with a comprehensive summary written by one of the editors, which includes input from the contributions as well as the editor's own thoughts on the subject. For all these reasons the book is well-suited as a primer to introduce graduate students in the richness of this field of research Astronomy, Observations and Techniques Astrophysics and Astroparticles Classical and Continuum Physics Observations, Astronomical Astronomy—Observations Astrophysics Continuum physics Interstellares Magnetfeld (DE-588)4137701-1 gnd rswk-swf Sternentstehung (DE-588)4057364-3 gnd rswk-swf Sternentstehung (DE-588)4057364-3 s Interstellares Magnetfeld (DE-588)4137701-1 s DE-604 Gómez de Castro, Ana I. edt Heyer, Mark edt Vázquez-Semadeni, Enrique edt Rebolo, Rafael edt Erscheint auch als Druck-Ausgabe 9789048166022 Erscheint auch als Druck-Ausgabe 9781402021596 Erscheint auch als Druck-Ausgabe 9789401704922 https://doi.org/10.1007/978-94-017-0491-5 Verlag URL des Erstveröffentlichers Volltext |
| spellingShingle | Magnetic Fields and Star Formation Theory Versus Observations Astronomy, Observations and Techniques Astrophysics and Astroparticles Classical and Continuum Physics Observations, Astronomical Astronomy—Observations Astrophysics Continuum physics Interstellares Magnetfeld (DE-588)4137701-1 gnd Sternentstehung (DE-588)4057364-3 gnd |
| subject_GND | (DE-588)4137701-1 (DE-588)4057364-3 |
| title | Magnetic Fields and Star Formation Theory Versus Observations |
| title_auth | Magnetic Fields and Star Formation Theory Versus Observations |
| title_exact_search | Magnetic Fields and Star Formation Theory Versus Observations |
| title_exact_search_txtP | Magnetic Fields and Star Formation Theory Versus Observations |
| title_full | Magnetic Fields and Star Formation Theory Versus Observations edited by Ana I. Gómez de Castro, Mark Heyer, Enrique Vázquez-Semadeni, Rafael Rebolo, Michel Tagger, Ralph E. Pudritz |
| title_fullStr | Magnetic Fields and Star Formation Theory Versus Observations edited by Ana I. Gómez de Castro, Mark Heyer, Enrique Vázquez-Semadeni, Rafael Rebolo, Michel Tagger, Ralph E. Pudritz |
| title_full_unstemmed | Magnetic Fields and Star Formation Theory Versus Observations edited by Ana I. Gómez de Castro, Mark Heyer, Enrique Vázquez-Semadeni, Rafael Rebolo, Michel Tagger, Ralph E. Pudritz |
| title_short | Magnetic Fields and Star Formation |
| title_sort | magnetic fields and star formation theory versus observations |
| title_sub | Theory Versus Observations |
| topic | Astronomy, Observations and Techniques Astrophysics and Astroparticles Classical and Continuum Physics Observations, Astronomical Astronomy—Observations Astrophysics Continuum physics Interstellares Magnetfeld (DE-588)4137701-1 gnd Sternentstehung (DE-588)4057364-3 gnd |
| topic_facet | Astronomy, Observations and Techniques Astrophysics and Astroparticles Classical and Continuum Physics Observations, Astronomical Astronomy—Observations Astrophysics Continuum physics Interstellares Magnetfeld Sternentstehung |
| url | https://doi.org/10.1007/978-94-017-0491-5 |
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