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Asteroseismology Across the HR Diagram: Proceedings of the Asteroseismology Workshop Porto, Portugal 1-5 July 2002 Softcover Repri Edition
Contributor(s): Thompson, Michael J. (Editor), Cunha, Margarida S. (Editor), Monteiro, Mario J. P. F. G. (Editor)
ISBN: 9048162416     ISBN-13: 9789048162413
Publisher: Springer
OUR PRICE:   $161.49  
Product Type: Paperback - Other Formats
Published: December 2010
Qty:
Additional Information
BISAC Categories:
- Science | Physics - Astrophysics
- Mathematics | Probability & Statistics - General
- Science | Astronomy
Dewey: 523.8
Physical Information: 0.66" H x 6.14" W x 9.21" (0.98 lbs) 294 pages
 
Descriptions, Reviews, Etc.
Publisher Description:
We stand at the threshold of an exciting era of Asteroseismology. In a few months' time, the Canadian small-satellite asteroseismology mission MOST will be laun- ched. Danish and French missions MONS and COROT should follow, with the ESA mission Eddington following in 2007/8. Helioseismology has proved spec- tacularly successful in imaging the internal structure and dynamics of the Sun and probing the physics of the solar interior. Ground-based observations have detected solar-like oscillations on alpha Centauri A and other Sun-like stars, and diagnostics similar to those used in helioseismology are now being used to test and constrain the physics and evolutionary state of these stars. Multi-mode oscillations are being observed in an abundance of other stars, including slowly pulsating B stars (SPB stars), delta Scuti stars, Ap stars and the pulsating white dwarfs. New classes of pulsators continue to be discovered across the Hertzsprung-Russell diagram. For good reason it was decided to entitle our conference 'Asteroseismology Across the HR Diagram' . Yet the challenges still to be faced to make asteroseismology across the HR diagram a reality are formidable. Observation, data analysis and theory all pose hard problems to be overcome. In conceiving this meeting, the aim of the organisers was to facilitate a cross-fertilization of ideas and approaches between researchers working on different pulsators and with different areas of expertise. We venture to suggest that in this the conference was a great success.