RGU photometry and population II stars

Details RGU photometry and population II stars RGU photometry and population II stars

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983a%26a...124..331t&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 124, no. 2, Aug. 1983, p. 331-333.

Astronomy and Astrophysics

Astrophysics

2

Stellar Color, Stellar Spectrophotometry, Metallicity

Scientific paper

Preliminary results on the calibration of the RGU photometric system in terms of atmospheric physical parameters are presented. Six stars with δ(U-G) excess are studied in three different fields: SA 54, SA 57, and M35. They are found metal deficient, in the range -0.6 ≤ [M/H]_sun;* ≤ -2.5. These results are consistent with the calibration of the RGU photometry based on synthetic spectra.

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