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Gravitational Dynamics
  • Language: en
  • Pages: 286

Gravitational Dynamics

Gravity plays a central role in the dynamics of all astrophysical systems - from stars to the Universe as a whole. This timely volume examines all aspects of gravitational dynamics - from stellar systems and galaxy disks, to the dynamics of the Local Group, large scale structures and motions, galaxy formation and general relativity. Each chapter is written by a world expert renowned for original contributions to the field. The authors are: James Binney, Roger Blandford, David Burstein, Tim de Zeeuw, George Efstathiou, Steve Gull, Nick Kaiser, J. Katz, Donald Lynden-Bell, Ruth Lynden-Bell, Douglas Lin, Jeremiah Ostriker, T. Padmanabhan, J. Papaloizou, Jim Peebles, Jim Pringle, Martin Rees, Maarteen Schmidt, Scott Tremaine and Simon White. This volume provides a broad, pedagogical introduction to gravitational dynamics for graduate students, and an up-to-date review for researchers in cosmology, astrophysics, mathematical physics and applied mathematics.

Gravitational Dynamics
  • Language: en

Gravitational Dynamics

  • Type: Book
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  • Published: 1996
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  • Publisher: Unknown

None

Cosmical Magnetism
  • Language: en
  • Pages: 222

Cosmical Magnetism

Prof. Leon Mestel has been an inspiration to many to study the role of magnetism in the Cosmos. To mark the occasion of his retin'ment from the University of Sussex after 43 years in astrophysics, several of his friends and former students decided to hold an advanced research workshop in his honour. NATO agreed to finance this venture which was held at the Institute of Astronomy at Cambridge. The scientific organizing committee was J. Landstreet, D. Lynden-Bell, F. Pacini, M.A. Rud0rman and N.O. Weiss and most leading experts on Cosmical magnetism agreed to come. We are particularly grateful to Lyman Spitzer who, ably helped by his wife Doreen, !!;ave the after dinner addre~s on how the godd...

Baryonic Dark Matter
  • Language: en
  • Pages: 301

Baryonic Dark Matter

The visible universe is a small perturbation on the material universe. Zwicky and Sinclair Smith in the 1930s gave evidence of invisible mass in the Coma and Virgo Clusters of Galaxies. Better optical data has only served to confound their critics and the X-ray data confirms that the gravitational potentials are many times larger than those predicted on the basis of the observed stars. Dynamical analyses of individual galaxies have found that significant extra mass is needed to explain their rotational velocities. On much larger scales, tens of megaparsecs, there is suggestive evidence that there is even more mass per unit luminosity. What is this non-luminous stuff of which the universe is made'? How much of it is there? Need there be only one kind of stuff? There are three basic possi bili ties:- all of it is ordinary (baryonic) matter, all of it is some other kind of (non-baryonic) matter, or some of it is baryonic and some is non-baryonic.

The Universe at Large
  • Language: en
  • Pages: 460

The Universe at Large

Eleven of the world's greatest living astronomers and cosmologists present their personal views of key problems in contemporary astronomy and cosmology.

The Woolley Symposium on the Galaxy and the Distance Scale
  • Language: en
  • Pages: 304

The Woolley Symposium on the Galaxy and the Distance Scale

  • Type: Book
  • -
  • Published: 1972
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  • Publisher: Unknown

None

Cosmical Magnetism
  • Language: en
  • Pages: 180

Cosmical Magnetism

  • Type: Book
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  • Published: 1994
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  • Publisher: Unknown

None

Dynamical Structure and Evolution of Stellar Systems
  • Language: en
  • Pages: 260

Dynamical Structure and Evolution of Stellar Systems

  • Type: Book
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  • Published: 1973
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  • Publisher: Unknown

None

The Structure and Evolution of Normal Galaxies
  • Language: en
  • Pages: 288

The Structure and Evolution of Normal Galaxies

None

Voyage to the Great Attractor
  • Language: en
  • Pages: 376

Voyage to the Great Attractor

  • Type: Book
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  • Published: 1994
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  • Publisher: Knopf

Dressler, an astronomer at the Observatories of the Carnegie Institution, tell the story of a decade-long study he undertook with six colleagues to determine whether the universe has expanded smoothly and symmetrically since its creation.