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：
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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.
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共 1386 条
[1]  
Adams FC(1987)Spectral evolution of young stellar objects Astrophys J 312 788-806
[2]  
Lada CJ(2001)The forbidden abundance of oxygen in the Sun Astrophys J Lett 556 L63-L66
[3]  
Shu FH(1993)Unified models for active galactic nuclei and quasars Annu Rev Astron Astrophys 31 473-521
[4]  
Allende Prieto C(1998)The navy prototype optical interferometer Astrophys J 496 550-597
[5]  
Lambert DL(2002)The application of interferometry to optical astronomical imaging Philos Trans R Soc Lond Ser A 360 969-229
[6]  
Asplund M(1986)Closure phase in high-resolution optical imaging Nature 320 595-945
[7]  
Antonucci R(1996)The first images from an optical aperture synthesis array: mapping of Capella with COAST at two epochs Astron Astrophys 306 213-1226
[8]  
Armstrong JT(2008)Image reconstruction at Cambridge University SPIE 7013 924-11
[9]  
Mozurkewich D(2003)Three-dimensional calculations of high- and low-mass planets embedded in protoplanetary discs Mon Not R Astron Soc 341 1221-1046
[10]  
Rickard LJ(1990)A survey for circumstellar disks around young stellar objects Astron J 99 7-1365
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