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Titlebook: Highlights of Spanish Astrophysics IV; Proceedings of the S Francesca Figueras,Josep Miquel Girart,Carme Jordi Conference proceedings 2007

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书目名称Highlights of Spanish Astrophysics IV
副标题Proceedings of the S
编辑Francesca Figueras,Josep Miquel Girart,Carme Jordi
视频video
图书封面Titlebook: Highlights of Spanish Astrophysics IV; Proceedings of the S Francesca Figueras,Josep Miquel Girart,Carme Jordi Conference proceedings 2007
描述.This volume documents the contributions presented at the Seventh Scientific Meeting of the Spanish Astronomical Society (Sociedad Española de Astronomía, SEA). The event bought together 301 participants who presented 161 contributed talks and 120 posters, the greatest numbers up to now. The fact that most exciting items of the current astronomical research were addressed in the meeting proofs the good health of the SEA, a consolidated organization founded fifteen years ago in Barcelona. Two plenary sessions of the meeting were devoted to the approved entrance of Spain as a full member of the European Southern Observatory (ESO) and to the imminent first light of the greatest telescope in the world, the GTC (Gran Telescopio de Canarias), milestones that will certainly lead the Spanish Astronomy in the next future. .
出版日期Conference proceedings 2007
关键词Accretion; Astrophysics; Cosmology; Dark matter; Galaxy; Plantary Science; Redshift; Solar Physics; Star; Uni
版次1
doihttps://doi.org/10.1007/978-1-4020-6000-7
isbn_softcover978-94-017-7665-3
isbn_ebook978-1-4020-6000-7
copyrightSpringer Science+Business Media B.V. 2007
The information of publication is updating

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OSIRIS: Status and Sciencefield of view, and capabilities for direct imaging, both long-slit and multiple object spectroscopy, and fast spectrophotometry. The combination of OSIRIS wide field, tunable filters plus charge shuffling array detectors, will constitute the most powerful instrument for studying faint emission-line
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The Star Formation History of Early-type Galaxies as a Function of Environmentronments. Using new models, that include a new and improved stellar library, we derive mean ages, metallicities and study the qualitative behaviour of different chemical elements. We conclude that more massive galaxies formed their stars on shorter time-scales than less massive ones. The formation e
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