Physics
Scientific paper
Aug 1999
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999noao.prop...11h&link_type=abstract
NOAO Proposal ID #1999B-0011
Physics
Scientific paper
We propose to initiate a three-year program at CTIO to determine parallaxes for stars in the solar neighborhood. The program will target faint, missing members of the nearby star sample --- primarily white, red and brown dwarfs. The results will allow us to improve the luminosities, colors, and temperatures for these common Galactic constituents, broaden the database used to investigate the luminosity function, mass function, kinematics, and multiplicity of stars in the solar neighborhood, estimate the age of the Galactic disk via the white dwarf luminosity function, and provide targets for upcoming extrasolar planetary searches. For this survey, nearby is defined as being within 20 parsecs, the horizon of NASA's NStars Project, which is a new initiative to provide high quality data for targets that will be observed in future space missions.
Anguita Claudio
Henry Todd
Ianna Phil
Mendez Rene
Ruiz María Teresa
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