Circumstellar disk

Results: 119



#Item
91Debris Disk Imaging
 with WFIRST-AFTA
 Geoff Bryden Jet Propulsion Laboratory,
 California Institute of Technology

Debris Disk Imaging
 with WFIRST-AFTA Geoff Bryden Jet Propulsion Laboratory, California Institute of Technology

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Source URL: exep.jpl.nasa.gov

Language: English - Date: 2014-07-01 12:26:02
92Microsoft Word - 20070810transcript.doc

Microsoft Word - 20070810transcript.doc

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Source URL: legacy.spitzer.caltech.edu

Language: English - Date: 2007-10-02 18:52:50
93JWST Science Questions From Gardner et al. 2006, Space Science Reviews. The End of the Dark Ages: First Light and Reionization The key objective of The End of the Dark Ages: First Light and Reionization theme is to ident

JWST Science Questions From Gardner et al. 2006, Space Science Reviews. The End of the Dark Ages: First Light and Reionization The key objective of The End of the Dark Ages: First Light and Reionization theme is to ident

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Source URL: jwst.nasa.gov

Language: English - Date: 2006-05-19 10:54:56
94Astronomy & Astrophysics A&A 533, A132[removed]DOI: [removed][removed]

Astronomy & Astrophysics A&A 533, A132[removed]DOI: [removed][removed]

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Source URL: aanda.u-strasbg.fr

Language: English
95Astronomy & Astrophysics A&A 533, A132[removed]DOI: [removed][removed]

Astronomy & Astrophysics A&A 533, A132[removed]DOI: [removed][removed]

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Source URL: www.aanda.org

Language: English
96Astronomy & Astrophysics A&A 533, A132[removed]DOI: [removed][removed]

Astronomy & Astrophysics A&A 533, A132[removed]DOI: [removed][removed]

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Source URL: cds.aanda.org

Language: English
97Contents 1 INTRODUCTION 2  2 OBSERVATIONAL CONSTRAINTS ON PLANET FORMATION THEORIES

Contents 1 INTRODUCTION 2 2 OBSERVATIONAL CONSTRAINTS ON PLANET FORMATION THEORIES

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Source URL: www.advanced-astronomy-guru-rupnathji.net63.net

Language: English - Date: 2013-02-21 04:22:50
98Abstract Flattened, rotating disks of cool dust and gas extending for tens to hundreds of AU are found around almost all low mass stars shortly after their birth. These disks generally persist for several Myr, during whi

Abstract Flattened, rotating disks of cool dust and gas extending for tens to hundreds of AU are found around almost all low mass stars shortly after their birth. These disks generally persist for several Myr, during whi

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Source URL: www.advanced-astronomy-guru-rupnathji.net63.net

Language: English - Date: 2013-02-21 03:19:17
99Initial Planetesimal Sizes and the Size Distribution of Small Kuiper Belt Objects

Initial Planetesimal Sizes and the Size Distribution of Small Kuiper Belt Objects

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Source URL: arxiv.org

Language: English - Date: 2013-04-02 20:40:19
100Variations on Debris Disks II. Icy Planet Formation as a Function of the Bulk Properties and Initial Sizes of Planetesimals

Variations on Debris Disks II. Icy Planet Formation as a Function of the Bulk Properties and Initial Sizes of Planetesimals

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Source URL: arxiv.org

Language: English - Date: 2010-04-13 21:42:45