Gravitational re-accumulation as the origin of most contact binaries and other small body shapes-Reference-Cited by-同舟云学术

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Gravitational re-accumulation as the origin of most contact binaries and other small body shapes

Published:2020-03 Issue: Volume:339 Page:113603
ISSN:0019-1035
Container-title:Icarus
language:en
Short-container-title:Icarus

Author:

Campo Bagatin Adriano,Alemañ Rafael A.,Benavidez Paula G.,Pérez-Molina Manuel,Richardson Derek C.

Funder

Spanish Ministerio de Economía, Industria y Competitividad

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference32 articles.

1. Near-infrared spectral results of asteroid Itokawa from the Hayabusa spacecraft;Abe;Science,2006

2. A comparison between rubble-pile and monolithic targets in impact simulations: Application to asteroid satellites and family size distributions;Benavidez;Icarus,2012

3. Dynamics of rotationally fissioned asteroids: non-planar case;Boldrin;Mon. Not. R. Astron. Soc.,2016

4. The YORP effect on 25143 Itokawa;Breiter;Astron. Astrophys.,2009

5. Internal structure of asteroid gravitational aggregates;Campo Bagatin;Icarus,2018

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