Low-Luminosity Main-Sequence Stars: NGC 6397 and the Solar Neighbourhood

Details Low-Luminosity Main-Sequence Stars: NGC 6397 and the Solar Neighbourhood Low-Luminosity Main-Sequence Stars: NGC 6397 and the Solar Neighbourhood

Apr 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aspc...92...76b&link_type=abstract

Formation of the Galactic Halo...Inside and Out, ASP Conference Series, Vol. 92, 1996, Heather Morrison and Ata Sarajedini, eds.

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5

Scientific paper

This is a preliminary report on low-mass stars. NGC 6397 HST data are compared with a solar-neighbourhood sample, confirming that metallicity plays a non-negligible role in determining the observed subdwarf distribution. New evolutionary computations of very-low-mass stars (VLM) are presented. The theoretical main sequence computed for metallicity feh = -1.91 shows very good agreement with the HST data of NGC 6397.

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