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What the Highest Angular Resolution Can Bring to Stellar Astrophysics? - - EDP Sciences

What the Highest Angular Resolution Can Bring to Stellar Astrophysics?

de F. Millour (rédacteur technique), A. Chiavassa (rédacteur technique), L. Bigot (rédacteur technique), O. Chesneau (rédacteur technique), A. Meilland (rédacteur technique), Ph. Stee (rédacteur technique)

Collection : EAS Publication Series

septembre 2015

Livre papier

format 1 x 1 388 pages En stock

70,00 €

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Présentation

This book contains lectures and tutorials offered to PhD students willing to learn the impact of stellar interferometry to its main scientific application : stellar physics. Indeed, stars are seen different, now that their surface or environments can be resolved by these incredibly complex systems that are long-baseline interferometers. Surface or environment images of a few targets start to be made, and will grow in the near-future with the advent of next generation imaging instruments.
The becoming of this book was impulsed by the VLTI school in the town of Barcelonnette in the french Alpes. The organization committee decided to write down the courses delivered during this very complete school of astrophysics. This book is dedicated to the memory of one of these organizers: Olivier Chesneau, who drived many stellar physics projects at the Observatoire de la Côte d’Azur, and who disappeared before being able to see the result of this work.

Compléments

Caractéristiques

Langue(s) : Anglais

Public(s) : Recherche

Editeur : EDP Sciences

Edition : 1^ère édition

Collection : EAS Publication Series

Publication : 15 septembre 2015

Référence Livre papier : L1833-4

EAN13 Livre papier : 9782759818334

Intérieur : Noir & blanc

Format (en mm) Livre papier : 1 x 1

Nombre de pages Livre papier : 388

Poids (en grammes) : 1

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