Strömgren photometry of the δ Sct star HR 4555

Details Strömgren photometry of the δ Sct star HR 4555 Strömgren photometry of the δ Sct star HR 4555

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009rmxac..35r.305r&link_type=abstract

XII Latin American IAU Regional Meeting (Eds. G. Magris, G. Bruzual, & L. Carigi) Revista Mexicana de Astronomía y Astrofísica (

Astronomy and Astrophysics

Astronomy

Scientific paper

We present preliminary results derived from the data obtained during three observing campaigns in 2000, 2001 and 2007, of the δ Sct-type variable star HR 4555, at Sierra Nevada Observatory, Spain. In all the cases, simultaneous uvbyβ photometry was carrried out. The analysis of the data was performed in the v band, by means of the Fourier Transform method, and results are shown. The intrinsic b-y, m_1 and c_1 values are derived and the physical parameters of this star are determined.

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