High-precision photometry with the WIRE satellite

Details High-precision photometry with the WIRE satellite High-precision photometry with the WIRE satellite

2005-09-15

arxiv.org/abs/astro-ph/0509444v1

Mem.Soc.Ast.It.77:278-281,2006

Astronomy and Astrophysics

Astrophysics

4 pages, conference proceedings, Workshop on Stellar Pulsation and Evolution, Rome, June 2005

Scientific paper

Around 200 bright stars (V < 6) have been monitored with the two-inch star
tracker on the WIRE satellite since observations started in 1999. Here we
present new results for the solar-like star Procyon A, the two Delta Scuti
stars Altair and Epsilon Cephei, and the triple system Lambda Scorpii which
consist of two B-type stars -- one of which we find to be an eclipsing binary.

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