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Cl* NGC 6522 ARP 1216 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.23CEST11:45:33 |
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 |
---|---|---|---|---|---|---|---|---|---|
1996AcA....46....1S | 1318 | 13 | The Optical Gravitational Lensing Experiment. The general catalog of stars in the Galactic Bulge. I. The stars in the central Baade's Window OGLE field BWC. | SZYMANSKI M., UDALSKI A., KUBIAK M., et al. | |||||
2008A&A...486..177Z | 15 | D | 1 | 531 | 293 | The metal content of bulge field stars from FLAMES-GIRAFFE spectra. I. Stellar parameters and iron abundances. | ZOCCALI M., HILL V., LECUREUR A., et al. | ||
2009ApJ...691.1387R | 15 | D | 1 | 3367 | 25 | Fabry-Perot absorption line spectroscopy of the Galactic bar. I. Kinematics. | RANGWALA N., WILLIAMS T.B. and STANEK K.Z. | ||
2009A&A...507..405B | 432 | D | X C | 11 | 47 | 24 | VLT-FLAMES analysis of 8 giants in the bulge metal-poor globular cluster NGC 6522: oldest cluster in the Galaxy? Analysis of 8 giants in NGC 6522. | BARBUY B., ZOCCALI M., ORTOLANI S., et al. | |
2011Natur.472..454C | 5 | 8 | 95 | Imprints of fast-rotating massive stars in the Galactic Bulge. | CHIAPPINI C., FRISCHKNECHT U., MEYNET G., et al. | ||||
2011A&A...529A.104C | 15 | D | 2 | 1347 | 2 | Coordinates and 2MASS and OGLE identifications for all stars in Arp's 1965 finding chart for Baade's Window. | CHURCH R.P., JOHNSON J.A. and FELTZING S. | ||
2014MNRAS.445.2994N | 16 | D | 4 | 11 | 14 | NGC 6522: a typical globular cluster in the Galactic bulge without signatures of rapidly rotating Population III stars. | NESS M., ASPLUND M. and CASEY A.R. | ||
2018A&A...614A.149D | 16 | D | 1 | 421 | 8 | Oxygen and zinc abundances in 417 Galactic bulge red giants. | DA SILVEIRA C.R., BARBUY B., FRIACA A.C.S., et al. | ||
2021A&A...654A..29B | 17 | D | 2 | 40 | 4 | UVES analysis of red giants in the bulge globular cluster NGC 6522. | BARBUY B., CANTELLI E., MUNIZ L., et al. |