Titlebook: White Dwarfs: Cosmological and Galactic Probes; Edward M. Sion,Stéphane Vennes,Harry L. Shipman Book 2005 Springer Science+Business Media

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Dark Halo Baryons not in Ancient White Dwarfs?ithin the magnitude-proper motion range, where such objects can be safely discriminated from any standard population..A robust range of scenarii for a galaxy halo, made of only 3 to 5% in mass of ancient white dwarfs, predicts the detection of 1 to 2 such objects in our survey, if the halo is at lea

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The Core/Envelope Symmetry in Pulsating White Dwarf Stars show how the signatures of composition transition zones brought about by physically distinct processes may be used to help alleviate this potential ambiguity in our asteroseismological interpretation of the pulsation frequencies.

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Type Ia Supernovae and Cosmologyge-scale structure surveys, we find a best fit for Ω. and Ω. of 0.28 and 0.72, respectively — essentially identical to the recent . results (and having comparable precision). The sum of the densities, ～ 1.0, agrees with extensive measurements of the cosmic microwave background radiation, including .

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0067-0057 they build upon...The book is suitable and most useful to advanced undergraduates, graduate students and scientific professionals (e.g. astronomers, astrophysicists, cosmologists, physicists). .978-90-481-6932-0978-1-4020-3725-2Series ISSN 0067-0057 Series E-ISSN 2214-7985

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C. Reylé,M. Crézé,V. Mohan,A. C. Robin,J.-C. Cuillandre,O. Le Fèvre,H. J. McCracken,Y. Mellier

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Stéphane Vennes,Adéla Kawka,Scott M. Croom,Brian J. Boyle,Robert J. Smith,Tom Shanks,Phil Outram,Lan

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