Asteroid clusters similar to asteroid pairs

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F18%3A00495453" target="_blank" >RIV/67985815:_____/18:00495453 - isvavai.cz</a>

Result on the web

<a href="http://dx.doi.org/10.1016/j.icarus.2017.08.008" target="_blank" >http://dx.doi.org/10.1016/j.icarus.2017.08.008</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1016/j.icarus.2017.08.008" target="_blank" >10.1016/j.icarus.2017.08.008</a>

Result language

angličtina

Original language name

Asteroid clusters similar to asteroid pairs

Original language description

We studied the membership, size ratio and rotational properties of 13 asteroid clusters consisting of between 3 and 19 known members that are on similar heliocentric orbits. By backward integrations of their orbits, we confirmed their cluster membership and estimated times elapsed since separation of the secondaries (the smaller cluster members) from the primary (i.e., cluster age) that are between 105 and a few 106 years.

Czech name

—

Czech description

—

Type

J_imp - Article in a specialist periodical, which is included in the Web of Science database

CEP classification

—

OECD FORD branch

10308 - Astronomy (including astrophysics,space science)

Project

Result was created during the realization of more than one project. More information in the Projects tab.

Continuities

P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Publication year

2018

Confidentiality

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Name of the periodical

Icarus

ISSN

1090-2643

e-ISSN

—

Volume of the periodical

304

Issue of the periodical within the volume

April

Country of publishing house

US - UNITED STATES

Number of pages

17

Pages from-to

110-126

UT code for WoS article

000426535800012

EID of the result in the Scopus database

2-s2.0-85028676596