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THE PROPER MOTION OF THE LARGE MAGELLANIC CLOUD REVISITED

The proper motion (PM) of the Large Magellanic Cloud (LMC) relative to four background quasi-stellar objects has been determined by reading and reprocessing image data from two previous studies. The total center of mass PM for the LMC obtained here is = (+1.94 ± 0.08) mas yr1, with a position angle...

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Publicat a:Revista Mexicana de Astronomía y Astrofísica
Autor principal: M. H. Pedreros
Format: Artigo
Idioma:Inglês
Publicat: Universidad Nacional Autónoma de México 2011
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Accés en línia:https://www.redalyc.org/articulo.oa?id=57120957011
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