The distance scale and the young blue populous cluster NGC 1866 in the LMC

Details The distance scale and the young blue populous cluster NGC 1866 in the LMC The distance scale and the young blue populous cluster NGC 1866 in the LMC

Jun 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ap%26ss.156...69s&link_type=abstract

(Instituto de Astrofisica de Canarias and Comision Interministerial de Ciencia y Tecnologia, Summer School on Evolutionary Pheno

Astronomy and Astrophysics

Astrophysics

B Stars, Blue Stars, Magellanic Clouds, Star Clusters, Stellar Spectrophotometry, Cepheid Variables, Charge Coupled Devices, H Beta Line, Interstellar Extinction, Light Curve, Metallicity

Scientific paper

The young blue populous cluster NGC 1866 in the LMC is an object which is well suited for a comparison of several basic distance indicators including ZAMS-fitting, the Cepheid period-luminosity relation, Baade-Wesselink analysis of the Cepheids and luminosity determination for the B-stars from Stromgren's uvby-H-beta photometry. A progress report on a project aimed at exploring these possibilities is presented here.

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