Charles P. Thompson; Douglas J. Herrmann; J. Don Read; Darryl Bruce; David G. Payne Taylor & Francis Ltd (2014) Saatavuus: Tilaustuote Pehmeäkantinen kirja
Charles P. Thompson; Douglas J. Herrmann; Darryl Bruce; J. Don Read; David G. Payne Taylor & Francis Inc (1997) Saatavuus: Tilaustuote Kovakantinen kirja
Charles P. Thompson; Douglas J. Herrmann; Darryl Bruce; J. Don Read; David G. Payne Taylor & Francis Ltd (2014) Saatavuus: Tilaustuote Pehmeäkantinen kirja
Charles P. Thompson; Douglas J. Herrmann; J. Don Read; Darryl Bruce; David G. Payne Taylor & Francis Inc (1997) Saatavuus: Tilaustuote Kovakantinen kirja
Charles W. Mitchell; Jean H. Baker; Richard Bell; Thomas G. Clemens; Robert J. Cook; Sharita Jacobs-Thompson; Marth Jones Louisiana State University Press (2021) Saatavuus: Tilaustuote Kovakantinen kirja
Springer Sivumäärä: 294 sivua Asu: Pehmeäkantinen kirja Julkaisuvuosi: 2010, 08.12.2010 (lisätietoa) Kieli: Englanti
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.