1996The Astronomical JournalRequires access

RR Lyrae Variable Stars in the CCD/Transit Instrument Survey

Charles J. Wetterer, J. T. McGraw, T. R. Hess, R. Grashuis

Open publisher page 13 citations

Abstract

We searched the CCD/Transit Instrument (CTI) survey databases for RR Lyrae variable stars. The CTI images a strip of the sky with a narrow spread of declination over all right ascensions. The resulting survey area covers a large range of both Galactic latitude and longitude, amounting to approximately 50 deg^2^. We detected a total of 42 RR Lyrae stars to a faint limiting magnitude of V = 19. Thirty-four of these RR Lyrae stars are newly discovered.

About this research paper

What this paper is about

We searched the CCD/Transit Instrument (CTI) survey databases for RR Lyrae variable stars. The CTI images a strip of the sky with a narrow spread of declination over all right ascensions. The resulting survey area covers a large range of both Galactic latitude and longitude, amounting to approximately 50 deg^2^. We detected a total of 42 RR Lyrae stars to a faint limiting magnitude of V = 19. Thirty-four of these RR Lyrae stars are newly discovered.

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Available abstract

We searched the CCD/Transit Instrument (CTI) survey databases for RR Lyrae variable stars. The CTI images a strip of the sky with a narrow spread of declination over all right ascensions. The resulting survey area covers a large range of both Galactic latitude and longitude, amounting to approximately 50 deg^2^. We detected a total of 42 RR Lyrae stars to a faint limiting magnitude of V = 19. Thirty-four of these RR Lyrae stars are newly discovered.

Key concepts: Physics, RR Lyrae variable, Variable star, Astronomy, Transit (satellite), Stars, Astrophysics, Globular cluster

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