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Origin of Elements in the Solar System
  • Language: en
  • Pages: 636

Origin of Elements in the Solar System

Based on an American Chemical Society Symposium organized by Professors Glenn Seaborg and Oliver Manuel, this volume provides a comprehensive record of different views on this important subject at the end of the 20th century. They have assembled a blend of highly respected experimentalists and theorists from astronomy, geology, meteoritics, planetology and nuclear chemistry and physics to discuss the origin of elements in the solar system. The intent was to include all points of view and let history judge their validity.

Challenges of asteroseismology in the era of space missions
  • Language: en
  • Pages: 157
Astrophysical Ages and Dating Methods
  • Language: en
  • Pages: 528

Astrophysical Ages and Dating Methods

None

Stellar Pulsations
  • Language: en
  • Pages: 285

Stellar Pulsations

Analyses of photometric time series obtained from the MOST, CoRoT and Kepler space missions were presented at the 20th conference on Stellar Pulsations (Granada, September 2011). These results are leading to a re-appraisal of our views on stellar pulsation in some stars and posing some new and unexpected challenges. The very important and exciting role played by innovative ground-based observational techniques, such as interferometric measurements of giant pulsating stars and high-resolution spectroscopy in the near infrared, is also discussed. These Proceedings are distinguished by the format of the conference, which brings together a variety of related but different topics not found in other meetings of this nature.

Publications of Los Alamos Research
  • Language: en
  • Pages: 210

Publications of Los Alamos Research

  • Type: Book
  • -
  • Published: 1987
  • -
  • Publisher: Unknown

None

Angular Momentum and Mass Loss for Hot Stars
  • Language: en
  • Pages: 366

Angular Momentum and Mass Loss for Hot Stars

Fundamental unsolved problems of stellar astrophysics include the effects of angular momentum on stellar structure and evolution, the nature and efficiency of the processes by which angular momentum is redistributed within and lost from stars, and the role that stellar rotation plays in enhancing or driving stellar mass loss. There appears to be a qualitative change in the nature and efficiency of these mechanisms near spectral type FO: hotter (more massive) stars typically retain more angular momentum at least until they reach the main sequence, while cooler stars typically spin down quickly. For the hotter stars, recent work suggests a strong link between the type of pulsation behavior, th...

Inside the Sun
  • Language: en
  • Pages: 509

Inside the Sun

Proceedings of the 121st Colloquium of the International Astronomical Union, held at Versailles, France, May 22-26, 1989

Physics at the Frontiers of the Standard Model
  • Language: en
  • Pages: 552