Lower main-sequence stars fundamental param. (Casagrande+, 2006)

Details Lower main-sequence stars fundamental param. (Casagrande+, 2006) Lower main-sequence stars fundamental param. (Casagrande+, 2006)

Jun 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ycat..73730013c&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/373/13. Originally published in: 2006MNRAS.373...13C

Physics

Stars: Dwarfs, Stars: Early-Type, Photometry, Effective Temperatures

Scientific paper

To recover accurate bolometric fluxes and temperatures for the stars, we have obtained accurate and homogeneous Johnson-Cousins BV(RI)C and JHKs photometry for all the 186 stars in our initial sample. For most of the stars in our sample with declination north of DE=-25°, we have made our own photometric observations from April to December 2004. Observations were done from Finland in full remote mode, using the 35-cm telescope piggybacked on the Swedish 60-cm telescope located at La Palma in the Canary Islands. A SBIG charge-coupled device was used through all the observations. Johnson-Cousins BV(RI)C colours were obtained for all stars. Infrared JHKs photometry for the sample has been taken from the Two-Micron All-Sky Survey (2MASS) catalogue.
(1 data file).

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