Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
11029466 | New Astronomy | 2019 | 14 Pages |
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
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Astronomy and Astrophysics
Authors
Derck P. Smits, P.L. Skelton,