Dynamical evolution of V-type asteroids in the central main belt-Reference-Cited by-同舟云学术

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Dynamical evolution of V-type asteroids in the central main belt

Published:2014-02-24 Issue:3 Volume:439 Page:3168-3179
ISSN:1365-2966
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Carruba V.,Huaman M. E.,Domingos R. C.,Santos C. R. Dos,Souami D.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/439/3/3168/13764493/stu192.pdf

Reference40 articles.

1. Iron meteorites as remnants of planetesimals formed in the terrestrial planet region

2. Mantle material in the main belt: Battered to bits?

3. The (not so) peculiar case of the Padua family

4. The stable archipelago in the region of the Pallas and Hansa dynamical families

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3. Gravitational study of escape routes and residence regions of Ceres and Vesta fragments;Astronomy & Astrophysics;2023-10

4. Igneous processes in the small bodies of the Solar System I. Asteroids and comets;iScience;2023-07

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