0
Your cart

Your cart is empty

Books > Science & Mathematics > Astronomy, space & time > Galaxies, clusters, intergalactic matter

Buy Now

Magnetic Fields and Star Formation - Theory Versus Observations (Hardcover, 2004 ed.) Loot Price: R4,662
Discovery Miles 46 620
Magnetic Fields and Star Formation - Theory Versus Observations (Hardcover, 2004 ed.): Ana I G omez de Castro, Mark Heyer,...

Magnetic Fields and Star Formation - Theory Versus Observations (Hardcover, 2004 ed.)

Ana I G omez de Castro, Mark Heyer, Enrique Vazquez-Semadeni, Rafael Rebolo, Michel Tagger, Ralph E. Pudritz

 (sign in to rate)
Loot Price R4,662 Discovery Miles 46 620 | Repayment Terms: R437 pm x 12*

Bookmark and Share

Expected to ship within 12 - 17 working days

Donate to Against Period Poverty

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.

General

Imprint: Springer-Verlag New York
Country of origin: United States
Release date: November 2004
First published: 2004
Editors: Ana I G omez de Castro • Mark Heyer • Enrique Vazquez-Semadeni • Rafael Rebolo • Michel Tagger • Ralph E. Pudritz
Dimensions: 235 x 155 x 28mm (L x W x T)
Format: Hardcover
Pages: 516
Edition: 2004 ed.
ISBN-13: 978-1-4020-2159-6
Categories: Books > Science & Mathematics > Astronomy, space & time > Galaxies, clusters, intergalactic matter > General
Books > Science & Mathematics > Physics > Applied physics & special topics > Astrophysics
LSN: 1-4020-2159-3
Barcode: 9781402021596

Is the information for this product incomplete, wrong or inappropriate? Let us know about it.

Does this product have an incorrect or missing image? Send us a new image.

Is this product missing categories? Add more categories.

Review This Product

No reviews yet - be the first to create one!

Partners