Spatial Distribution of the High-Velocity Clouds

Details Spatial Distribution of the High-Velocity Clouds Spatial Distribution of the High-Velocity Clouds

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009rmxac..35...72o&link_type=abstract

XII Latin American IAU Regional Meeting (Eds. G. Magris, G. Bruzual, & L. Carigi) Revista Mexicana de Astronomía y Astrofísica (

Astronomy and Astrophysics

Astronomy

Galaxies: Interactions, Galaxies: Magellanic Clouds, Galaxy: Halo, Ism: Clouds

Scientific paper

I developed a method to determine theoretical distances to the High-Velocity Clouds (HVCs), based on the idea that the HVCs were ejected from the Magellanic Clouds in a relatively short period of time as a consequence of the collision between the Large (LMC) and Small Magellanic Clouds (SMC). The present spatial position of each HVCs was obtained by calculating its orbit with the initial condition that the each HVCs was simultaneously launched from the LMC at the time and position of the LMC-SMC encounter.

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