Hostname: page-component-8448b6f56d-m8qmq Total loading time: 0 Render date: 2024-04-19T03:32:36.236Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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