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Temporal evolution of coronagraphic dynamic range and constraints on companions to Vega

S Hinkley, BR Oppenheimer, R Soummer… - The Astrophysical …, 2007 - iopscience.iop.org
The major obstacle to the direct detection of companions to nearby stars is the
overwhelming brightness of the host star. Current instruments employing the combination of …
被引用次数：170 相关文章
[PDF] academia.edu

[PDF][PDF] Temporal Evolution of Coronagraphic Dynamic Range, and Constraints on Companions to Vega

S Hinkley, BR Oppenheimer, R Soummer… - arXiv preprint astro-ph … - academia.edu
The major obstacle to the direct detection of companions to nearby stars is the
overwhelming brightness of the host star. Current instruments employing the combination of …
[PDF] psu.edu

[PDF][PDF] Temporal Evolution of Coronagraphic Dynamic Range, and Constraints on Companions to Vega

S Hinkley, BR Oppenheimer, R Soummer… - arXiv preprint astro-ph … - Citeseer
The major obstacle to the direct detection of companions to nearby stars is the
overwhelming brightness of the host star. Current instruments employing the combination of …

Temporal Evolution of Coronagraphic Dynamic Range, and Constraints on Companions to Vega

S Hinkley, BR Oppenheimer, R Soummer… - arXiv preprint astro-ph …, 2006 - arxiv.org
The major obstacle to the direct detection of companions to nearby stars is the
overwhelming brightness of the host star. Current instruments employing the combination of …

[引用][C] Temporal Evolution of Coronagraphic Dynamic Range and Constraints on Companions to Vega

S Hinkley, BR Oppenheimer, R Soummer… - The Astrophysical …, 2007 - cir.nii.ac.jp
Temporal Evolution of Coronagraphic Dynamic Range and Constraints on Companions to
Vega | CiNii Research CiNii 国立情報学研究所 学術情報ナビゲータ[サイニィ] 詳細へ移動 検索 …
[PDF] core.ac.uk

[PDF][PDF] Temporal Evolution of Coronagraphic Dynamic Range, and Constraints on Companions to Vega

S Hinkley, BR Oppenheimer, R Soummer… - arXiv preprint astro-ph …, 2006 - core.ac.uk
The major obstacle to the direct detection of companions to nearby stars is the
overwhelming brightness of the host star. Current instruments employing the combination of …

Temporal Evolution of Coronagraphic Dynamic Range, and Constraints on Companions to Vega

S Hinkley, BR Oppenheimer, R Soummer… - Astrophys. J., 2006 - inspirehep.net
The major obstacle to the direct detection of companions to nearby stars is the
overwhelming brightness of the host star. Current instruments employing the combination of …
[PDF] archive.org

[PDF][PDF] Temporal Evolution of Coronagraphic Dynamic Range, and Constraints on Companions to Vega

S Hinkley, BR Oppenheimer, R Soummer… - arXiv preprint astro …, 2006 - scholar.archive.org
The major obstacle to the direct detection of companions to nearby stars is the
overwhelming brightness of the host star. Current instruments employing the combination of …

Temporal Evolution of Coronagraphic Dynamic Range and Constraints on Companions to Vega

S Hinkley, BR Oppenheimer… - The Astrophysical …, 2007 - ui.adsabs.harvard.edu
The major obstacle to the direct detection of companions to nearby stars is the
overwhelming brightness of the host star. Current instruments employing the combination of …

[引用][C] Temporal evolution of coronagraphic dynamic range and constraints on companions to vega

S HINKLEY, BR OPPENHEIMER… - The Astrophysical …, 2007 - pascal-francis.inist.fr
Temporal evolution of coronagraphic dynamic range and constraints on companions to
vega CNRS Inist Pascal-Francis CNRS Pascal and Francis Bibliographic Databases Simple …