Asteroids’ physical models from combined dense and sparse photometry and scaling of the YORP effect by the observed obliquity distribution
about
An anisotropic distribution of spin vectors in asteroid familiesNew and updated convex shape models of asteroids based on optical data from a large collaboration networkAsteroid models from the Lowell photometric databaseAsteroid shapes and thermal properties from combined optical and mid-infrared photometry inversionVolumes and bulk densities of forty asteroids from ADAM shape modelingThe non-convex shape of (234) Barbara, the first Barbarian*
P2860
Asteroids’ physical models from combined dense and sparse photometry and scaling of the YORP effect by the observed obliquity distribution
description
2013 թուականի Փետրուարին հրատարակուած գիտական յօդուած
@hyw
2013 թվականի փետրվարին հրատարակված գիտական հոդված
@hy
article publié dans la revue scientifique Astronomy and Astrophysics
@fr
artículu científicu espublizáu en 2013
@ast
im Februar 2013 veröffentlichter wissenschaftlicher Artikel
@de
scientific article (publication date: 22 February 2013)
@en
wetenschappelijk artikel (gepubliceerd op 2013/02/22)
@nl
наукова стаття, опублікована в лютому 2013
@uk
مقالة علمية (نشرت في 22-2-2013)
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name
Asteroids’ physical models fro ...... bserved obliquity distribution
@ast
Asteroids’ physical models fro ...... bserved obliquity distribution
@en
type
label
Asteroids’ physical models fro ...... bserved obliquity distribution
@ast
Asteroids’ physical models fro ...... bserved obliquity distribution
@en
prefLabel
Asteroids’ physical models fro ...... bserved obliquity distribution
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Asteroids’ physical models fro ...... bserved obliquity distribution
@en
P2093
P50
P356
P1476
Asteroids’ physical models fro ...... bserved obliquity distribution
@en
P2093
A. Cazenave
A. Coupier
A. Kryszczyńska
A. Laffont
A. Oksanen
P356
10.1051/0004-6361/201220701
P407
P50
P577
2013-02-22T00:00:00Z
P5875
P818
P819
2013A&A...551A..67H