UBV photometry of HR 1176

Details UBV photometry of HR 1176 UBV photometry of HR 1176

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ap%26ss.162..337d&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 162, no. 2, Dec. 1989, p. 337-340.

Astronomy and Astrophysics

Astrophysics

Astronomical Photometry, F Stars, G Stars, Light Curve, Stellar Spectra, Ubv Spectra, Emission Spectra, K Stars, Line Spectra, Radial Velocity

Scientific paper

This paper presents photoelectric UBV observations of the suspected Ca II emission line star HR 1176. A period analysis of the observations by using the method of Shell-Metzner failed to yield any true period which is probably due to the large gaps in the observations, low-amplitude variation, and the nonconstancy of the period, or there may be no regular light variation. A visual inspection of the present observations shows no systematic or abrupt variability except some scatter. However, a long period eclipsing nature of HR 1176 cannot be ruled out.

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