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Faint optical spiral tracers

Published online by Cambridge University Press:  14 August 2015

Juan C. Muzzio*
Affiliation:
Observatorio Astronómico de la Universidad Nacional de La Plata, and Consejo Nacional de Investigaciones Científicas y Técnicas de la República Argentina

Extract

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The use of modern photographic emulsions and techniques allows for the discovery of optical spiral tracers much fainter than was possible in the past. Our searches for such faint objects deal with the Puppis, Vela, Crux, Circinus, Norma and Ara regions of the Milky Way using Kodak plates (baked in dry nitrogen) obtained with the Curtis Schmidt-telescope at Cerro Tololo Inter-American Observatory. We have discovered OB stars as faint as 15 mag on IIIa-J plates obtained with the thin prism, and Hα emission-line objects (many of which are Be stars) as faint as 16 mag on 127-04 plates obtained with the 4° prism.

Type
II. THE DISK COMPONENT
Copyright
Copyright © Reidel 1979