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dc.date.accessioned 2019-10-17T15:34:11Z
dc.date.available 2019-10-17T15:34:11Z
dc.date.issued 2004
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/83503
dc.description.abstract The majority of the high-velocity clouds (HVC) having a common origin linked to the dynamic evolution of the Magellanic Clouds was discussed. It was concluded that the HVC surround the Galaxy, forming a metacloud of ∼300 kpc in size and with a mass of ∼3×109 M⊙. It was found that the HVC were the product of a powerful superwind, which occurred in the Magellanic Clouds about 570 Myr ago as a consequence of the interaction of the Large and Small Magellanic Clouds. The effects of the passage of the HVC flow through the Galactic disk produced on the interstellar medium were also analyzed. en
dc.format.extent 895-907 es
dc.language en es
dc.subject Galaxies: interactions es
dc.subject Galaxies: Magellanic Clouds es
dc.subject Galaxy: evolution es
dc.subject Galaxy: halo es
dc.subject Galaxy: structure es
dc.subject ISM: clouds es
dc.title The high-velocity clouds and the Magellanic Clouds en
dc.type Articulo es
sedici.identifier.other http://dx.doi.org/10.1051/0004-6361:20040177 es
sedici.identifier.issn 0004-6361 es
sedici.creator.person Olano, Carlos Alberto es
sedici.subject.materias Ciencias Astronómicas es
sedici.description.fulltext true es
mods.originInfo.place Facultad de Ciencias Astronómicas y Geofísicas es
sedici.subtype Articulo es
sedici.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/
sedici.description.peerReview peer-review es
sedici.relation.journalTitle Astronomy and Astrophysics es
sedici.relation.journalVolumeAndIssue vol. 423, no. 3 es


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Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Except where otherwise noted, this item's license is described as Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)