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| CD-48 14210 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST19:34:48 |
Sort references on where and how often the object is cited
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 |
|---|---|---|---|---|---|---|---|---|---|
| 1965IBVS...86....1S | 20 | 8 | Bright southern BV stars. | STROHMEIER W., KNIGGE R. and OTT H. | |||||
2004yCat.2250....0S 
|
3358 | 107 | Combined General Catalogue of Variable Stars. | SAMUS N.N. and DURLEVICH O.V. | |||||
|
2017AJ....153..257O
|
16 | D | 1 | 10625 | 142 | Comoving stars in Gaia DR1: an abundance of very wide separation comoving pairs. | OH S., PRICE-WHELAN A.M., HOGG D.W., et al. | ||
|
2017MNRAS.472..675A
|
16 | D | 1 | 13582 | 89 | Wide binaries in Tycho-Gaia: search method and the distribution of orbital separations. | ANDREWS J.J., CHANAME J. and AGUEROS M.A. | ||
|
2018A&A...609A.116R
|
16 | D | 1 | 143018 | 65 | Empirical photometric calibration of the Gaia red clump: Colours, effective temperature, and absolute magnitude. | RUIZ-DERN L., BABUSIAUX C., ARENOU F., et al. | ||
|
2018AJ....155..149B
|
16 | D | 1 | 9764 | 5 | Fundamental properties of co-moving stars observed by Gaia. | BOCHANSKI J.J., FAHERTY J.K., GAGNE J., et al. | ||
|
2021ApJ...921..118N
|
17 | D | 2 | 70 | 14 | Distant relatives: the chemical homogeneity of comoving pairs identified in Gaia. | NELSON T., TING Y.-S., HAWKINS K., et al. | ||
|
2022MNRAS.514.1071M
|
17 | D | 1 | 2315 | ~ | A measurement of stellar surface gravity hidden in radial velocity differences of comoving stars. | MOSCHELLA M., SLONE O., DROR J.A., et al. | ||
|
2024Natur.627..501L
|
18 | D | 1 | 246 | ~ | At least one in a dozen stars shows evidence of planetary ingestion. | LIU F., TING Y.-S., YONG D., et al. | ||
| 2026A&A...707L...2P | 20 | D | 3 | 49 | ~ | Wide binaries without viable bound Newtonian orbits. | PASQUINI L., SAGLIA R., PATAT F., et al. |
