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Astronomy at high angular resolution...

Boffin, Henri M.J.

Astronomy at high angular resolutiona compendium of techniques in the visible and near-infrared /

Record Type:	Electronic resources : Monograph/item
Title/Author:	Astronomy at high angular resolutionedited by Henri M.J. Boffin ... [et al.].
Reminder of title:	a compendium of techniques in the visible and near-infrared /
other author:	Boffin, Henri M.J.
Published:	Cham :Springer International Publishing :2016.
Description:	xvi, 274 p. :ill., digital ;24 cm.
Contained By:	Springer eBooks
Subject:	Astrotomography.
Online resource:	http://dx.doi.org/10.1007/978-3-319-39739-9
ISBN:	9783319397399$q(electronic bk.)

Astronomy at high angular resolutiona compendium of techniques in the visible and near-infrared /
Astronomy at high angular resolutiona compendium of techniques in the visible and near-infrared /[electronic resource] :edited by Henri M.J. Boffin ... [et al.]. - Cham :Springer International Publishing :2016. - xvi, 274 p. :ill., digital ;24 cm. - Astrophysics and space science library,4390067-0057 ;. - Astrophysics and space science library ;379..

Introduction by the editors -- Adaptive optics -- Aperture masking imaging -- Disentangling of stellar spectra -- Interferometry -- Lucky Imaging -- Roche tomography -- Spectro-astrometry -- Astrotomography of planets -- Adaptive optics of planets & disks -- Stellar surfaces with interferometry -- The Galactic Centre at high-angular resolution -- AGN interferometry -- AGN reverberation mapping -- Doppler and Magnetic Imaging of Stellar Surfaces -- Doppler Tomography -- Doppler Tomography of Polars -- Doppler Imaging of cool stars and brown dwarfs -- Eclipse Mapping -- Stokes Imaging.

This book offers an essential compendium of astronomical high-resolution techniques. Recent years have seen considerable developments in such techniques, which are critical to advances in many areas of astronomy. As reflected in the book, these techniques can be divided into direct methods, interferometry, and reconstruction methods, and can be applied to a huge variety of astrophysical systems, ranging from planets, single stars and binaries to active galactic nuclei, providing angular resolution in the micro- to tens of milliarcsecond scales. Written by experts in their fields, the chapters cover adaptive optics, aperture masking imaging, spectra disentangling, interferometry, lucky imaging, Roche tomography, imaging with interferometry, interferometry of AGN, AGN reverberation mapping, Doppler- and magnetic imaging of stellar surfaces, Doppler tomography, eclipse mapping, Stokes imaging, and stellar tomography. This book is intended to enable a next generation of astronomers to apply high-resolution techniques. It informs readers on how to achieve the best angular resolution in the visible and near-infrared regimes from diffraction-limited to micro-arcsecond scales.

ISBN: 9783319397399$q(electronic bk.)

Standard No.: 10.1007/978-3-319-39739-9doiSubjects--Topical Terms:

742373
Astrotomography.

LC Class. No.: QB51.3.I45

Dewey Class. No.: 522.6

Astronomy at high angular resolutiona compendium of techniques in the visible and near-infrared /
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505 0 $a Introduction by the editors -- Adaptive optics -- Aperture masking imaging -- Disentangling of stellar spectra -- Interferometry -- Lucky Imaging -- Roche tomography -- Spectro-astrometry -- Astrotomography of planets -- Adaptive optics of planets & disks -- Stellar surfaces with interferometry -- The Galactic Centre at high-angular resolution -- AGN interferometry -- AGN reverberation mapping -- Doppler and Magnetic Imaging of Stellar Surfaces -- Doppler Tomography -- Doppler Tomography of Polars -- Doppler Imaging of cool stars and brown dwarfs -- Eclipse Mapping -- Stokes Imaging.
520 $a This book offers an essential compendium of astronomical high-resolution techniques. Recent years have seen considerable developments in such techniques, which are critical to advances in many areas of astronomy. As reflected in the book, these techniques can be divided into direct methods, interferometry, and reconstruction methods, and can be applied to a huge variety of astrophysical systems, ranging from planets, single stars and binaries to active galactic nuclei, providing angular resolution in the micro- to tens of milliarcsecond scales. Written by experts in their fields, the chapters cover adaptive optics, aperture masking imaging, spectra disentangling, interferometry, lucky imaging, Roche tomography, imaging with interferometry, interferometry of AGN, AGN reverberation mapping, Doppler- and magnetic imaging of stellar surfaces, Doppler tomography, eclipse mapping, Stokes imaging, and stellar tomography. This book is intended to enable a next generation of astronomers to apply high-resolution techniques. It informs readers on how to achieve the best angular resolution in the visible and near-infrared regimes from diffraction-limited to micro-arcsecond scales.
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