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| Cl* NGC 2168 SB 231 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.23CEST20:33:30 |
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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 |
|---|---|---|---|---|---|---|---|---|---|
| 1971AJ.....76..475C | 336 | 34 | Relative proper motions in the region of the open cluster NGC 2168 (M 35). | CUDWORTH K.M. | |||||
| 1986AJ.....91..557M | 430 | 25 | A proper-motion analysis of the cluster M 35. | McNAMARA B. and SEKIGUCHI K. | |||||
1999MNRAS.306..361S 
|
1160 | 76 | UBVI CCD photometry of M 35 (NGC 2168). | SUNG H. and BESSELL M.S. | |||||
|
2001ApJ...546.1006B
|
15 | D | 1937 | 64 | From the top to the bottom of the main sequence: a complete mass function of the young open cluster M35. | BARRADO Y NAVASCUES D., STAUFFER J.R., BOUVIER J., et al. | |||
|
2009ApJ...695..679M
|
15 | D | 1 | 452 | 193 | Stellar rotation in M35: mass-period relations, spin-down rates, and gyrochronology. | MEIBOM S., MATHIEU R.D. and STASSUN K.G. | ||
|
2010AJ....139.1383G
|
15 | D | 1 | 1159 | 33 | WIYN open cluster study. XXXVIII. Stellar radial velocities in the young open cluster M35 (NGC 2168). | GELLER A.M., MATHIEU R.D., BRADEN E.K., et al. | ||
|
2011AJ....141...89S
|
15 | D | 1 | 1053 | 146 | The SEGUE stellar parameter pipeline. IV. Validation with an extended sample of galactic globular and open clusters. | SMOLINSKI J.P., LEE Y.S., BEERS T.C., et al. | ||
|
2015MNRAS.448..822X
|
16 | D | 1 | 188 | 130 | The LAMOST stellar parameter pipeline at Peking University - LSP3. | XIANG M.S., LIU X.W., YUAN H.B., et al. | ||
|
2015AJ....150...10L
|
16 | D | 1 | 1361 | 6 | WIYN open cluster study. LXVI. Spectroscopic binary orbits in the young open cluster M35 (NGC 2168). | LEINER E.M., MATHIEU R.D., GOSNELL N.M., et al. | ||
|
2020ApJS..246...15S
|
17 | D | 1 | 1164 | ~ | A catalog of periodic variables in open clusters M35 and NGC 2158. | SOARES-FURTADO M., HARTMAN J.D., BHATTI W., et al. |
