Binary paths to type Ia supernovae explosions : proceedings of the 281st Symposium of the International Astronomical Union, held in Padova, Italy, July 4-8, 2011 /

Reviews recent progress in theory and observations which lead to a wider range of possible progenitor models than ever before. Presents all sides of the ongoing debates, while retaining a diversity of opinions on a wide range of topics reflecting physical uncertainties relating to the Type Ia progen...

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Bibliographic Details
Corporate Authors: International Astronomical Union. Symposium
Group Author: Di Stefano, Rosanne Gloria; Orio, M. Marina; Moe, Maxwell
Published: Cambridge University Press,
Publisher Address: Cambridge, United Kingdom ; New York, NY, USA :
Publication Dates: 2013.
Literature type: Book
Language: English
Series: IAU symposium proceedings series,
Subjects:
Summary: Reviews recent progress in theory and observations which lead to a wider range of possible progenitor models than ever before. Presents all sides of the ongoing debates, while retaining a diversity of opinions on a wide range of topics reflecting physical uncertainties relating to the Type Ia progenitor puzzle. The 2011 Nobel Prize for Physics was awarded to three astrophysicists who inferred the existence of dark energy from Type Ia supernova data.
Carrier Form: xxvii, 353 pages : illustrations ; 26 cm.
Bibliography: Includes bibliographical references and index.
ISBN: 9781107019812 :
1107019818
CLC: P145.3-532
Call Number: P145.3-532/I612-1/2011
Contents: Survey : new perspectives on cosmology and the type Ia supernova progenitor problem -- Stellar & binary processes: Single and binary star evolution ; The role of rotation -- Cataclysmic variables and classical novae -- Possible progenitors of type Ia supernovae: Nuclear burning white dwarfs ; Recurrent novae and symbiotics ; Helium doners ; Double white dwarfs ; Population synthesis -- New insights on SNe Ia progenitors from their explosions and aftermath: Explosion physics ; Signatures of progenitors in light curves & spectra ; Signatures of progenetors in supernova remnants -- Summary: Bin