Lyman-alpha as an Astrophysical and Cosmological Tool, 1st ed. 2019 Saas-Fee Advanced Course 46. Swiss Society for Astrophysics and Astronomy Saas-Fee Advanced Course Series, Vol. 46
Auteurs : Dijkstra Mark, Prochaska J. Xavier, Ouchi Masami, Hayes Matthew
Coordonnateurs : Verhamme Anne, North Pierre, Cantalupo Sebastiano, Atek Hakim
The hydrogen Lyman-alpha line is of utmost importance to many fields of astrophysics. This UV line being conveniently redshifted with distance to the visible and even near infrared wavelength ranges, it is observable from the ground, and provides the main observational window on the formation and evolution of high redshift galaxies. Absorbing systems that would otherwise go unnoticed are revealed through the Lyman-alpha forest, Lyman-limit, and damped Lyman-alpha systems, tracing the distribution of baryonic matter on large scales, and its chemical enrichment.
Dr. Pierre North is senior researcher and lecturer at the Laboratory of Astrophysics of the Ecole Polytechnique Fédérale de Lausanne (EPFL). He obtained his PhD degree in astronomy and astrophysics in 1984 at Geneva University. He worked on chemically peculiar stars, especially on the evolution of the angular momentum of magnetic Ap and Bp stars. He studied the rate and properties of binaries among this type of stars, and also determined the orbital and spectral properties of Ba dwarfs, to the discovery of which he contrib
Fills a gap of graduate lecture books dedicated to this topic
Gathers state-of-the art theory and observations
Discusses main science case of several forthcoming facilities
Presents elaborated lecture notes of the 46th Saas-Fee Advanced Course
Date de parution : 11-2020
Ouvrage de 403 p.
15.5x23.5 cm
Disponible chez l'éditeur (délai d'approvisionnement : 15 jours).
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Ajouter au panierDate de parution : 11-2019
Ouvrage de 403 p.
15.5x23.5 cm