LMC massive star clusters R 127 & R 128 resolved

Details LMC massive star clusters R 127 & R 128 resolved LMC massive star clusters R 127 & R 128 resolved

Jun 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002sf2a.conf..541m&link_type=abstract

SF2A-2002: Semaine de l'Astrophysique Francaise, meeting held in Paris, France, June 24-29, 2002, Eds.: F. Combes and D. Barret,

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Scientific paper

We study the Large Magellanic Cloud star clusters R 127 and R 128 using imaging and spectroscopy obtained at the ESO NTT telescope. An advanced image restoration technique allows us to resolve and obtain photometry of initially unresolved components, while medium dispersion spectroscopy allows us to identify the LBV component and the types of several other hot stars belonging to the cluster.

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