Astrometry and Photometry of Open Clusters: NGC 1746, NGC 1750 and NGC 1758

Details Astrometry and Photometry of Open Clusters: NGC 1746, NGC 1750 and NGC 1758 Astrometry and Photometry of Open Clusters: NGC 1746, NGC 1750 and NGC 1758

Jun 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998ap%26ss.263..307g&link_type=abstract

Astrophysics and Space Science, v. 263, Issue 1/4, p. 307-310 (1998).

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

We present an astrometric and photometric analysis of a 5 square degree region around NGC 1746, NGC 1750 and NGC 1758, close to the Galactic anti-center (l = 179°, b = -10°), in Taurus. We describe the acquisition, reduction and analysis of the observational data, including the development of innovative data analysis tools. The data comprise CCD UBVRI photometry, photographic BVR photometry and proper motions.

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