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Asteroseismology Across the HR Diagram - Proceedings of the Asteroseismology Workshop Porto, Portugal 1-5 July 2002 (Hardcover, 2003 ed.) Loot Price: R4,739
Discovery Miles 47 390
Asteroseismology Across the HR Diagram - Proceedings of the Asteroseismology Workshop Porto, Portugal 1-5 July 2002 (Hardcover,...

Asteroseismology Across the HR Diagram - Proceedings of the Asteroseismology Workshop Porto, Portugal 1-5 July 2002 (Hardcover, 2003 ed.)

Michael J. Thompson, Margarida S. Cunha, Mario J.P.F.G. Monteiro

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Loot Price R4,739 Discovery Miles 47 390 | Repayment Terms: R444 pm x 12*

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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."

General

Imprint: Springer-Verlag New York
Country of origin: United States
Release date: May 2003
First published: 2003
Editors: Michael J. Thompson • Margarida S. Cunha • Mario J.P.F.G. Monteiro
Dimensions: 235 x 155 x 19mm (L x W x T)
Format: Hardcover
Pages: 294
Edition: 2003 ed.
ISBN-13: 978-1-4020-1173-3
Categories: Books > Science & Mathematics > Astronomy, space & time > Galaxies, clusters, intergalactic matter > General
Books > Science & Mathematics > Physics > Applied physics & special topics > Astrophysics
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LSN: 1-4020-1173-3
Barcode: 9781402011733

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