Rotation of the Milky Way and the Formation of the Magellanic Stream
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F11%3A00425515" target="_blank" >RIV/67985815:_____/11:00425515 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1051/eas/1148076" target="_blank" >http://dx.doi.org/10.1051/eas/1148076</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1051/eas/1148076" target="_blank" >10.1051/eas/1148076</a>
Alternative languages
Result language
angličtina
Original language name
Rotation of the Milky Way and the Formation of the Magellanic Stream
Original language description
We studied the impact of the revisited values for the LSR circular velocity of the Milky Way (Reid et al. 2004) on the formation of the Magellanic Stream. The LSR circular velocity was varied within its observational uncertainties as a free parameter ofthe interaction between the Large (LMC) and the Small (SMC) Magellanic Clouds and the Galaxy. We have shown that the large scale morphology and kinematics of the Magellanic Stream may be reproduced as tidal features, assuming the recent values of the proper motions of the Magellanic Clouds (Kallivayalil et al. 2006).
Czech name
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Czech description
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Classification
Type
D - Article in proceedings
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
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Result continuities
Project
—
Continuities
Z - Vyzkumny zamer (s odkazem do CEZ)
Others
Publication year
2011
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Article name in the collection
CRAL-2010: A Universe of Dwarf Galaxies
ISBN
9782759806621
ISSN
1633-4760
e-ISSN
—
Number of pages
7
Pages from-to
337-343
Publisher name
EDP Sciences
Place of publication
Les Ulis
Event location
Lyon
Event date
Jun 14, 2010
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
000308567700076