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| IC 4756 88 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST07:11:05 |
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trying to find the most relevant references on this object.
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 |
|---|---|---|---|---|---|---|---|---|---|
| 1943AN....274...69K | 503 | 46 | Untersuchung der offenen Sternhaufen IC 4665, NGC 6633, IC 4756. | KOPFF E. | |||||
| 1975A&AS...19..211H | 90 | 41 | Membership and photometry of the open cluster IC 4756. | HERZOG A.D., SANDERS W.L. and SEGGEWISS W. | |||||
1995AJ....109.1903M 
|
90 | 4 | Amendment of our method for deriving stellar membership of an open cluster. | MISSANA M. and MISSANA N. | |||||
|
2007AJ....134.1216J
|
39 | 37 | Na, al, and O abundances of open clusters NGC 7142, NGC 6939, and IC 4756. | JACOBSON H.R., FRIEL E.D. and PILACHOWSKI C.A. | |||||
|
2018A&A...615A..49C
|
16 | D | 1 | 224763 | 54 | Characterising open clusters in the solar neighbourhood with the Tycho-Gaia Astrometric Solution. | CANTAT-GAUDIN T., VALLENARI A., SORDO R., et al. | ||
|
2019MNRAS.490.2521H
|
16 | D | 1 | 6544 | ~ | Fractal statistics in young star clusters: structural parameters and dynamical evolution. | HETEM A. and GREGORIO-HETEM J. | ||
|
2020A&A...633A..99C
|
16 | D | 1 | 257585 | 169 | Clusters and mirages: cataloguing stellar aggregates in the Milky Way. | CANTAT-GAUDIN T. and ANDERS F. | ||
|
2020A&A...640A...1C
|
16 | D | 1 | 235399 | 241 | Painting a portrait of the Galactic disc with its stellar clusters. | CANTAT-GAUDIN T., ANDERS F., CASTRO-GINARD A., et al. | ||
|
2022ApJ...931..156P
|
17 | D | 1 | 22106 | 16 | 3D Morphology of Open Clusters in the Solar Neighborhood with Gaia EDR 3. II. Hierarchical Star Formation Revealed by Spatial and Kinematic Substructures. | PANG X., TANG S.-Y., LI Y., et al. | ||
|
2022ApJS..262....7H
|
17 | D | 1 | 134735 | 19 | A Blind All-sky Search for Star Clusters in Gaia EDR3: 886 Clusters within 1.2 kpc of the Sun. | HE Z., WANG K., LUO Y., et al. |
