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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| Vydáno v: | Revista Mexicana de Astronomía y Astrofísica |
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| Hlavní autor: | |
| Médium: | Artigo |
| Jazyk: | Inglês |
| Vydáno: |
Universidad Nacional Autónoma de México
2011
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| Témata: | |
| On-line přístup: | https://www.redalyc.org/articulo.oa?id=57120957011 |
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