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| 2MASS J00241513-7204365 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST21:55:26 |
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| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 1995MNRAS.276..739M | 1 | 9 | 62 | IR-array photometry of galactic globular clusters - II. JK photometry of 47 Tuc. | MONTEGRIFFO P., FERRARO F.R., FUSI PECCI F., et al. | ||||
| 1996ApJ...464L.157E | 1 | 12 | 82 | K giants in 47 Tucanae: detection of a new class of variable stars. | EDMONDS P.D. and GILLILAND R.L. | ||||
| 2004A&A...424..199B | 2 | 20 | 127 | The calibration of the RGB Tip as a Standard Candle. Extension to Near Infrared colors and higher metallicity. | BELLAZZINI M., FERRARO F.R., SOLLIMA A., et al. | ||||
| 2005A&A...441.1117L | 47 | 63 | Long period variables in 47 Tuc: direct evidence for lost mass. | LEBZELTER T. and WOOD P.R. | |||||
| 2011ApJ...730...71M | 167 | D | X | 5 | 28 | 33 | Dust production and mass loss in the galactic globular cluster 47 Tucanae. | McDONALD I., BOYER M.L., VAN LOON J.Th., et al. | |
2011ApJS..193...23M 
|
129 | D | X | 4 | 48 | 48 | Fundamental parameters, integrated red giant branch mass loss, and dust production in the galactic globular cluster 47 Tucanae. | McDONALD I., BOYER M.L., VAN LOON J.Th., et al. | |
|
2012A&A...537A...2M
|
15 | D | 2 | 110 | 17 | The VLT/VISIR mid-IR view of 47 Tucanae. A further step in solving the puzzle of RGB mass loss. | MOMANY Y., SAVIANE I., SMETTE A., et al. | ||
| 2012A&A...540A..32G | 15 | D | 1 | 146 | 20 | Infrared excess around nearby red giant branch stars and Reimers law. | GROENEWEGEN M.A.T. | ||
| 2018A&A...618A..58M | 16 | D | 1 | 89645 | 72 | Gaia Data Release 2. The first Gaia catalogue of long-period variable candidates. | MOWLAVI N., LECOEUR-TAIBI I., LEBZELTER T., et al. | ||
| 2024A&A...688A...9S | 18 | D | 1 | 91 | ~ | “Forbidden” stars in the eROSITA all-sky survey: X-ray emission from very late-type giants. | SCHMITT J.H.M.M., HUNSCH M., SCHNEIDER P.C., et al. |
