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Velocity fields in late-type galaxies from H-alpha Fabry-Perot interferometry. I - Instrumentation and data reduction

G. de Vaucouleurs, W. D. Pence

Open publisher page 14 citations

Abstract

An image-tube H-alpha Fabry-Perot interferometer used for the mapping of velocity fields in late-type galaxies with the Galaxymeter at McDonald Observatory is described. The semiautomated method of reduction leading to the construction of detailed velocity maps at 4 to 10 arcsec resolution from 500 to 5000 velocities per galaxy is outlined. Accidental and systematic errors are discussed.

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What this paper is about

An image-tube H-alpha Fabry-Perot interferometer used for the mapping of velocity fields in late-type galaxies with the Galaxymeter at McDonald Observatory is described. The semiautomated method of reduction leading to the construction of detailed velocity maps at 4 to 10 arcsec resolution from 500 to 5000 velocities per galaxy is outlined. Accidental and systematic errors are discussed.

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Available abstract

An image-tube H-alpha Fabry-Perot interferometer used for the mapping of velocity fields in late-type galaxies with the Galaxymeter at McDonald Observatory is described. The semiautomated method of reduction leading to the construction of detailed velocity maps at 4 to 10 arcsec resolution from 500 to 5000 velocities per galaxy is outlined. Accidental and systematic errors are discussed.

Key concepts: Physics, Galaxy, Astrophysics, Astronomy, Data reduction, Astronomical interferometer, Astrometry, Interferometry

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