CCD photometry of Galactic clusters containing Cepheid variables. I - Lynga 6

Details CCD photometry of Galactic clusters containing Cepheid variables. I - Lynga 6 CCD photometry of Galactic clusters containing Cepheid variables. I - Lynga 6

Apr 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985mnras.213..889w&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 213, April 15, 1985, p. 889-897.

Astronomy and Astrophysics

Astronomy

60

Cepheid Variables, Color-Magnitude Diagram, Galactic Clusters, Astronomical Photometry, Charge Coupled Devices

Scientific paper

A color-magnitude diagram has been derived for the Galactic cluster Lynga 6, on the basis of CCD photometric observations carried out using the SAAO-UCL CCD camera on the 1.0-m Sutherland telescope. The photometric accuracy observations was near 0.01 mag at V = 19-20. The true distance modulus for Lynga 6 is estimated, yielding a value of 11.5 + or - 0.3. Estimates of the magnitude in violet of the 10.8-day Cepheid variable TW Nor yielded a value of (Mv) = 3.8 + or - 0.3. TW Nor appears to be a member of the Lynga 6 cluster. An identification chart of the cluster is provided.

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