Can eccentric debris disks be long-lived? - Wikidata - awgldk - TriplyDB

Can eccentric debris disks be long-lived?

Can eccentric debris disks be long-lived?

http://www.wikidata.org/entity/Q56445347

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Near-infrared scattered light properties of the HR 4796 A dust ring Azimuthal asymmetries in the debris disk around HD 61005A massive collision of planetesimals?

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Can eccentric debris disks be long-lived?

http://www.wikidata.org/entity/Q56445347

description

article publié dans la revue scientifique Astronomy and Astrophysics

@fr

im März 2014 veröffentlichter wissenschaftlicher Artikel

@de

scientific article published in Astronomy and Astrophysics

@en

wetenschappelijk artikel

@nl

наукова стаття, опублікована в березні 2014

@uk

name

Can eccentric debris disks be long-lived?

@en

Can eccentric debris disks be long-lived?

@nl

type

label

Can eccentric debris disks be long-lived?

@en

Can eccentric debris disks be long-lived?

@nl

prefLabel

Can eccentric debris disks be long-lived?

@en

Can eccentric debris disks be long-lived?

@nl

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Astronomy and Astrophysics

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Can eccentric debris disks be long-lived?

@en

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A. Mora

http://www.w3.org/2001/XMLSchema#string

B. Montesinos

http://www.w3.org/2001/XMLSchema#string

C. Eiroa

http://www.w3.org/2001/XMLSchema#string

C. del Burgo

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G. Bryden

http://www.w3.org/2001/XMLSchema#string

G. J. White

http://www.w3.org/2001/XMLSchema#string

H. Beust

http://www.w3.org/2001/XMLSchema#string

J. Milli

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J. P. Marshall

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J.-C. Augereau

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Optical images of an exosolar planet 25 light-years from Earth

Direct imaging of multiple planets orbiting the star HR 8799

Validation of the new Hipparcos reduction

A Jupiter-mass companion to a solar-type star

Contributions to the Nearby Stars (NStars) Project: Spectroscopy of Stars Earlier than M0 within 40 pc--The Southern Sample

Search for associations containing young stars (SACY)

The Origin of Pluto's Orbit: Implications for the Solar System Beyond Neptune

Debris Disks around Sun‐like Stars

A new algorithm for self-consistent three-dimensional modeling of collisions in dusty debris disks

A planetary system as the origin of structure in Fomalhaut's dust belt.

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72–72

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scholarly article

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10.1051/0004-6361/201322469

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563

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2014-03-01T00:00:00Z

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259346857

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1312.5146

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2014A&A...563A..72F

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