Physical properties of asteroid dust bands and their sources
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F06%3A00003194" target="_blank" >RIV/00216208:11320/06:00003194 - isvavai.cz</a>
Result on the web
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DOI - Digital Object Identifier
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Alternative languages
Result language
angličtina
Original language name
Physical properties of asteroid dust bands and their sources
Original language description
Disruptive collisions in the main belt can liberate fragments from parent bodies ranging in size from several micrometers to tens of kilometers in diameter.
Czech name
Fyzikální vlastnosti asteroidálních prachových pásů a jejich zdroje
Czech description
Kolize asteroidů v hlavním pásu uvolňují fragmenty velikosti sub-mikronů do kilometrů.
Classification
Type
J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
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Result continuities
Project
<a href="/en/project/GA205%2F05%2F2737" target="_blank" >GA205/05/2737: The Yarkovsky and YORP effects in translational and rotational motion of asteroids</a><br>
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)
Others
Publication year
2006
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
Icarus : International Journal of Solar System Studies
ISSN
0019-1035
e-ISSN
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Volume of the periodical
181
Issue of the periodical within the volume
1
Country of publishing house
MX - MEXICO
Number of pages
38
Pages from-to
107-144
UT code for WoS article
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EID of the result in the Scopus database
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