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Abstract Variable stars in HLF 356 identified from plates taken at Harvard Observatory southern station in the 1930s are characterised using data from the ASAS, SuperWASP and Catalina Sky Survey… Click to show full abstract
Abstract Variable stars in HLF 356 identified from plates taken at Harvard Observatory southern station in the 1930s are characterised using data from the ASAS, SuperWASP and Catalina Sky Survey databases. Very little work has been done on these variables since their discovery. Their periods are determined, and light curves for these stars are presented, from which their classification is determined.
Keywords:
characterization eclipsing;
binaries high;
latitude field;
eclipsing binaries;
field 356;
high latitude
Journal Title: New Astronomy
Year Published: 2019
Link to full text (if available)
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Journal Title: New Astronomy
Year Published: 2019
Link to full text (if available)
Share on Social Media: Sign Up to like & get
recommendations!