| Download | - View final version: A photometric study of the outer halo globular cluster NGC 5824 (PDF, 4.4 MiB)
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| DOI | Resolve DOI: https://doi.org/10.3847/1538-3881/aa72f9 |
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| Author | Search for: Walker, A. R.; Search for: Andreuzzi, G.; Search for: Martínez-Vázquez, C. E.; Search for: Kunder, A. M.; Search for: Stetson, P. B.1; Search for: Cassisi, S.; Search for: Monelli, M.; Search for: Bono, G.; Search for: Dall’ora, M; Search for: Vivas, A. K. |
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| Affiliation | - National Research Council of Canada. Herzberg Astronomy and Astrophysics
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| Format | Text, Article |
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| Subject | galaxy: stellar content; stars: distance; stars: evolution; stars: horizontal-brand; stars: population II |
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| Abstract | Multi-wavelength CCD photometry over 21 years has been used to produce deep color–magnitude diagrams (CMDs) together with light curves for the variables in the Galactic globular cluster NGC 5824. Twenty-one new cluster RR Lyrae stars are identified, bringing the total to 47, of which 42 have reliable periods determined for the first time. |
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| Publication date | 2017-06-13 |
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| Publisher | American Astronomical Society |
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| In | |
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| Language | English |
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| Peer reviewed | Yes |
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| NPARC number | 23002578 |
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| Export citation | Export as RIS |
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| Report a correction | Report a correction (opens in a new tab) |
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| Record identifier | 7ea40b99-7c00-4fb9-aa4b-f693968d0378 |
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| Record created | 2017-12-01 |
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| Record modified | 2020-05-30 |
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