[PLH2002] CX5 , the SIMBAD biblio

[PLH2002] CX5 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST12:59:49


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Title First 3 Authors
2001PASP..113..764D viz 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.
2003ApJ...595..179F 1 18 65 The puzzling dynamical status of the core of the globular cluster NGC 6752. FERRARO F.R., POSSENTI A., SABBI E., 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 viz 286       D S   X C F     5 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 422       D     X C       10 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 888       D S   X C       19 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.
2023ApJ...944..225L 47           X         1 141 ~ A Comparison of Millisecond Pulsar Populations between Globular Clusters and the Galactic Field. LEE J., HUI C.Y., TAKATA J., et al.
2024ApJ...964L..20R 50           X         1 253 ~ Reevaluating the Origin of Detectable Cataclysmic Variables in Globular Clusters: Testing the Importance of Dynamics. RIVERA SANDOVAL L., BELLONI D. and RAMOS AREVALO M.

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