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New variables in the Large Magellanic Cloud
Published online by Cambridge University Press: 14 August 2015
Extract
This work was performed in the same way as that corresponding to the Small Cloud (Landi Dessy 1959a, 1959b). Two hundred and seventy-seven new variables have been discovered, whose positions are shown by arrows in Figure 1. The pairs of plates used for blinking have from 80m to more than 1000d intervals.
- Type
- Section II: The Magellanic Clouds
- Information
- Symposium - International Astronomical Union , Volume 20: The Galaxy and the Magellanic Clouds , 1964 , pp. 377 - 380
- Copyright
- Copyright © Australian Academy of Science 1964
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