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| Cl* NGC 4590 SAW V12 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST21:14:28 |
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More on score
| Bibcode/DOI | Score |
in Title|Abstract| Keywords |
in a table | in teXt, Caption, ... | Nb occurence | Nb objects in ref |
Citations (from ADS) |
Title | First 3 Authors |
|---|---|---|---|---|---|---|---|---|---|
| 1920ApJ....51...49S | 29 | 6 | Studies based on the colors and magnitudes in stellar clusters. XV. A photometric analysis of the globular cluster system Messier 68. | SHAPLEY H. | |||||
1994AJ....107..622B 
|
28 | 18 | CCD photometry of RR Lyrae stars in the globular cluster M 68. | BROCATO E., CASTELLANI V. and RIPEPI V. | |||||
|
2004A&A...421..937G
|
64 | 102 | Metal abundances of RR Lyrae stars in the bar of the Large Magellanic Cloud. | GRATTON R.G., BRAGAGLIA A., CLEMENTINI G., et al. | |||||
| 2014NewA...27...56S | 93 | D | C | 2 | 53 | 3 | Variable stars in the globular cluster NGC 4590 (M68). | SARIYA D.P., LATA S. and YADAV R.K.S. | |
|
2015A&A...578A.128K
|
328 | D | X C | 8 | 67 | 15 | A census of variability in globular cluster M 68 (NGC 4590). | KAINS N., ARELLANO FERRO A., FIGUERA JAIMES R., et al. | |
|
2019A&A...622A..60C
|
16 | D | 1 | 150347 | 194 | Gaia Data Release 2. Specific characterisation and validation of all-sky Cepheids and RR Lyrae stars. | CLEMENTINI G., RIPEPI V., MOLINARO R., et al. | ||
|
2022MNRAS.510.3575H
|
17 | D | 1 | 71780 | 1 | Identifying RR Lyrae in the ZTF DR3 data set. | HUANG K.-W. and KOPOSOV S.E. | ||
|
2023ApJ...944...88L
|
17 | D | 1 | 135907 | 6 | Photometric Metallicity and Distance Estimates for ∼136,000 RR Lyrae Stars from Gaia Data Release 3. | LI X.-Y., HUANG Y., LIU G.-C., et al. | ||
|
2023A&A...674A..18C
|
17 | D | 1 | 271810 | 30 | Gaia Data Release 3 Specific processing and validation of all-sky RR Lyrae and Cepheid stars: The RR Lyrae sample. | CLEMENTINI G., RIPEPI V., GAROFALO A., et al. | ||
|
2024A&A...690L..17L
|
18 | D | 1 | 11379 | ~ | An 'alien' called the Oosterhoff dichotomy? | LUONGO E., RIPEPI V., MARCONI M., et al. |
