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Crowded Field Electronography in the LMC

Published online by Cambridge University Press:  04 August 2017

Peter Linde ,
Arne Ardeberg ,
Harri Lindgren  and
Gösta Lyngå
Peter Linde
Affiliation:
Lund Observatory, Box 1107, S-221 04 Lund, Sweden AA and HL also at ESO, La Silla, Chile
Arne Ardeberg
Affiliation:
Lund Observatory, Box 1107, S-221 04 Lund, Sweden AA and HL also at ESO, La Silla, Chile
Harri Lindgren
Affiliation:
Lund Observatory, Box 1107, S-221 04 Lund, Sweden AA and HL also at ESO, La Silla, Chile
Gösta Lyngå
Affiliation:
Lund Observatory, Box 1107, S-221 04 Lund, Sweden AA and HL also at ESO, La Silla, Chile

Extract

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An area in the LMC situated 1.2 degrees from the centre of the Bar has been studied with the ESO 3.6 m telescope using electronography and photoelectric measurements for calibration. Coordinates for 1950.0 are 5h20m, −71°. Six exposures have been used, with exposure times ranging from 8 to 90 min. Typical seeing was 1.5 arcseconds FWHM. This investigation is a continuation of our earlier study with the ESO 1.5 m telescope (Lindgren et al., 1980).

Type
Evolution
Information
Symposium - International Astronomical Union , Volume 108: Structure and Evolution of the Magellanic Clouds , 1984 , pp. 99 - 100
Copyright
Copyright © Reidel 1984 

References

Lindgren, H., Ardeberg, A., Linde, P., Lyngå, G.: 1980, in ESO Workshop on two dimensional photometry, Noordwijkerhout, p. 155 Google Scholar
Stryker, L.L., Butcher, H.R.: 1981, in IAU Colloquium No. 68, Schenectady, N.Y., p. 255 Google Scholar