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HD 3242


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A photometric study of wide visual double stars. IV - UVBY photometry of wide visual double stars with G-type primaries
We performed uvby aperture photometry of wide visual double stars withG-type primaries. The minimum angular separation of the components is 10arcsecs and mainly less than 20 arcsecs. As both components have oftensimilar photometric and astrophysical parameters, we infer that most ofthese double stars have components of common origin.

The Energy Distribution in Lyman Continuum and the Effective Temperatures of Planetary Nebulae Nuclei
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A second list of wide visual binaries
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A second list of wide visual binaries
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Observation and Astrometry data

Constellation:Pisces
Right ascension:00h35m37.39s
Declination:+03°19'18.0"
Apparent magnitude:9.021
Proper motion RA:-11.7
Proper motion Dec:-25.6
B-T magnitude:10.232
V-T magnitude:9.121

Catalogs and designations:
Proper Names   (Edit)
HD 1989HD 3242
TYCHO-2 2000TYC 13-1459-1
USNO-A2.0USNO-A2 0900-00139270

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