Fitted UBV magnitude for MS stars (Naylor+, 2009)

Details Fitted UBV magnitude for MS stars (Naylor+, 2009) Fitted UBV magnitude for MS stars (Naylor+, 2009)

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ycat..73990432n&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/399/432. Originally published in: 2009MNRAS.399..432N

Computer Science

Models, Clusters: Open, Stars: Early-Type, Photometry: Ubv

Scientific paper

To compare a set of ages derived from MS evolution with contraction ages, we need a sample of clusters and associations which have contraction ages, and for each of which data are available for MS fitting. Our sample is, therefore, based on the groups we placed in age order using the PMS in Mayne & Naylor (2008MNRAS.386..261M).
(2 data files).

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