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From Interacting Binaries to Exoplanets (IAU S282): Essential Modeling Tools (Proceedings of the International Astronomical Union Symposia and Colloquia)

Mercedes T. Richards , Ivan Hubeny

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ISBN 10: 1107019826 / ISBN 13: 9781107019829
Editorial: Cambridge University Press, 2012
Usado Condición: Very Good Encuadernación de tapa dura
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Ex-library but minimal markings only on ffep & edge of pages, Book is tight & clean/unmarked, barely opened & a very nice book otherwise ! Size: 4to - over 9¾" - 12" tall. N° de ref. de la librería 033546

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Detalles bibliográficos

Título: From Interacting Binaries to Exoplanets (IAU...

Editorial: Cambridge University Press

Año de publicación: 2012

Encuadernación: Hard Cover

Condición del libro: Very Good

Condición de la sobrecubierta: No Jacket

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Sinopsis:

In IAU Symposium 282, members of the exoplanet and binary star communities unite for the first time to discuss the state-of-the-art discovery, imaging, modeling and analysis tools used to study stars, brown dwarfs and exoplanets in multiple-object systems. They describe detection techniques using advanced telescopes and detectors, including the Kepler mission and the proposed Gaia and LSST projects. Imaging techniques discussed include adaptive optics, interferometry, polarimetry and tomography, while key modeling tools are covered in detail. Other topics include simulations of formation mechanisms in binary star systems, non-conservative evolution of binary stars, the formation and evolution of planets and a theory for the structure, atmospheres and evolution of giant exoplanets. The volume concludes with hydrodynamic simulations, models of planetary atmospheres and the habitability of exoplanets. These proceedings demonstrate how sophisticated modeling codes bridge the gap between theory and observations and increase our understanding of binary and multiple systems.

Book Description:

IAU 282 is the product of the first official symposium to unite members of the exoplanet and binary star communities. Researchers discuss the state-of-the-art tools used to study stars, brown dwarfs and exoplanets in multiple-object systems and demonstrate how sophisticated modeling codes bridge the gap between theory and observations.

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