Imaging the heart of astrophysical objects with optical long-baseline interferometry

被引：0

作者：

J.-P. Berger

F. Malbet

F. Baron

A. Chiavassa

G. Duvert

M. Elitzur

B. Freytag

F. Gueth

S. Hönig

J. Hron

H. Jang-Condell

J.-B. Le Bouquin

J.-L. Monin

J. D. Monnier

G. Perrin

B. Plez

T. Ratzka

S. Renard

S. Stefl

E. Thiébaut

K. R. W. Tristram

T. Verhoelst

S. Wolf

J. Young

机构：

[1] Université J. Fourier (Grenoble 1),CNRS, UMR 5571, Institut de Planétologie et d’Astrophysique de Grenoble

[2] European Southern Observatory,Cavendish Laboratory

[3] University of Michigan,Centre de Recherche en Astrophysique de Lyon, UMR 5574

[4] University of Cambridge,Department of Physics

[5] Max-Planck-Institut für Astrophysik,Institut für Astronomie

[6] Jean Marie Mariotti Center,Department of Physics & Astronomy 1000 E.

[7] University of Kentucky,Laboratoire d’Etudes Spatiales et d’Instrumentation en Astrophysique, UMR 8109

[8] Université de Lyon/École Normale Supérieure de Lyon/CNRS,Laboratoire Univers et Particules de Montpellier, UMR 5299

[9] Institut de Radioastronomie Millimétrique,Institute of Astronomy

[10] Max-Planck-Institut für Radioastronomie,Institut d’Astronomie et d’Astrophysique

[11] University of California in Santa Barbara,undefined

[12] Universität Wien,undefined

[13] University of Wyoming,undefined

[14] Observatoire de Paris/CNRS,undefined

[15] CNRS,undefined

[16] Universitäts-Sternwarte München,undefined

[17] KULeuven,undefined

[18] University of Kiel,undefined

[19] Université Libre de Bruxelles,undefined

来源：

The Astronomy and Astrophysics Review | 2012年 / 20卷

关键词：

Instrumentation: interferometers; Techniques: interferometric; Methods: data processing; Planetary systems: protoplanetary disks; Stars: supergiants; Stars: AGB—circumstellar matter; Stars: imaging; Galaxies: active; Galaxies nuclei;

D O I：

暂无

中图分类号：

学科分类号：

摘要：

The number of publications of aperture-synthesis images based on optical long-baseline interferometry measurements has recently increased due to easier access to visible and infrared interferometers. The interferometry technique has now reached a technical maturity level that opens new avenues for numerous astrophysical topics requiring milli-arcsecond model-independent imaging. In writing this paper our motivation was twofold: (1) review and publicize emblematic excerpts of the impressive corpus accumulated in the field of optical interferometry image reconstruction; (2) discuss future prospects for this technique by selecting four representative astrophysical science cases in order to review the potential benefits of using optical long-baseline interferometers.

引用

共 50 条

[1] Imaging the heart of astrophysical objects with optical long-baseline interferometry
Berger, J. -P.
Malbet, F.
Baron, F.
Chiavassa, A.
Duvert, G.
Elitzur, M.
Freytag, B.
Gueth, F.
Hoenig, S.
Hron, J.
Jang-Condell, H.
Le Bouquin, J. -B.
Monin, J. -L.
Monnier, J. D.
Perrin, G.
Plez, B.
Ratzka, T.
Renard, S.
Stefl, S.
Thiebaut, E.
Tristram, K. R. W.
Verhoelst, T.
Wolf, S.
Young, J.
[J]. ASTRONOMY AND ASTROPHYSICS REVIEW, 2012, 20 : 1 - 55
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Le Besnerais, Guy
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[3] Imaging "Pinwheel" nebulae with optical long-baseline interferometry
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