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| [JVH94] NGC 6752 22 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.23CEST07:32:55 |
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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 |
|---|---|---|---|---|---|---|---|---|---|
| 2000A&A...358..910V | 71 | 27 | Multiple and variable X-ray sources in the globular clusters ω Cen, NGC 6397, NGC 6752, and Liller 1. | VERBUNT F. and JOHNSTON H.M. | |||||
2001PASP..113..764D 
|
1714 | 277 | A catalog and atlas of cataclysmic variables: the living edition. | DOWNES R.A., WEBBINK R.F., SHARA M.M., et al. | |||||
| 2002ApJ...569..405P | 35 | 79 | Optical identification of multiple faint X-ray sources in the globular cluster NGC 6752: evidence for numerous cataclysmic variables. | POOLEY D., LEWIN W.H.G., HOMER L., et al. | |||||
| 2008MNRAS.388.1111P | 38 | X | 1 | 122 | 10 | Cluster AgeS Experiment (CASE): deficiency of observed dwarf novae in globular clusters. | PIETRUKOWICZ P., KALUZNY J., SCHWARZENBERG-CZERNY A., et al. | ||
|
2012MNRAS.423.2901T
|
325 | D | S X C F | 6 | 21 | 8 | A multiwavelength survey of NGC 6752: X-ray counterparts, two new dwarf novae and a core-collapsed radial profile. | THOMSON G.S., KNIGGE C., DIEBALL A., et al. | |
| 2014MNRAS.441..757F | 94 | D | F | 3 | 84 | 13 | A Chandra look at the X-ray faint millisecond pulsars in the globular cluster NGC 6752. | FORESTELL L.M., HEINKE C.O., COHN H.N., et al. | |
| 2017ApJ...841...53L | 301 | D | X | 8 | 41 | 3 | Identification of faint Chandra X-ray sources in the core-collapsed globular cluster NGC 6752. | LUGGER P.M., COHN H.N., COOL A.M., et al. | |
| 2018MNRAS.475.4841R | 16 | D | 1 | 114 | 34 | New cataclysmic variables and other exotic binaries in the globular cluster 47 Tucanae*. | RIVERA SANDOVAL L.E., VAN DEN BERG M., HEINKE C.O., et al. | ||
| 2021MNRAS.508.2823C | 322 | D | S X | 7 | 58 | 5 | A deep search for faint Chandra X-ray sources, radio sources, and optical counterparts in NGC 6752. | COHN H.N., LUGGER P.M., ZHAO Y., et al. |
