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| ESO-HA 405 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST03:59:28 |
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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 |
|---|---|---|---|---|---|---|---|---|---|
2004AJ....127.1117R 
|
366 | 18 | Hα emission-line stars in molecular clouds. I. The NGC 2264 region. | REIPURTH B., PETTERSSON B., ARMOND T., et al. | |||||
|
2004AJ....128.1684S
|
3054 | 45 | The initial mass function and young brown dwarf candidates in NGC 2264. I. The initial mass function around S Monocerotis. | SUNG H., BESSELL M.S. and CHUN M.-Y. | |||||
|
2005AJ....129..829D
|
522 | 114 | The T Tauri star population of the young cluster NGC 2264. | DAHM S.E. and SIMON T. | |||||
|
2013MNRAS.429.1981B
|
16 | D | 1 | 595 | 9 | Bayesian inference of T Tauri star properties using multi-wavelength survey photometry. | BARENTSEN G., VINK J.S., DREW J.E., et al. | ||
|
2013ApJS..209...32B
|
16 | D | 1 | 8196 | 71 | Identifying young stars in massive star-forming regions for the MYStIX project. | BROOS P.S., GETMAN K.V., POVICH M.S., et al. | ||
|
2014ApJ...794..124R
|
16 | D | 1 | 599 | 5 | A Spitzer view of the giant molecular cloud Mon OB1 EAST/NGC 2264. | RAPSON V.A., PIPHER J.L., GUTERMUTH R.A., et al. | ||
|
2014A&A...570A..82V
|
16 | D | 1 | 770 | 103 | Mapping accretion and its variability in the young open cluster NGC 2264: a study based on u-band photometry. | VENUTI L., BOUVIER J., FLACCOMIO E., et al. | ||
|
2015A&A...581A..66V
|
16 | D | 1 | 683 | 36 | UV variability and accretion dynamics in the young open cluster NGC 2264. | VENUTI L., BOUVIER J., IRWIN J., et al. | ||
| 2020A&A...636A..80B | 17 | D | 1 | 175 | ~ | The spatial evolution of young massive clusters. II. Looking for imprints of star formation in NGC 2264 with Gaia DR2. | BUCKNER A.S.M., KHORRAMI Z., GONZALEZ M., et al. | ||
|
2021MNRAS.503.3279S
|
17 | D | 1 | 104619 | 56 | The GALAH survey: tracing the Galactic disc with open clusters. | SPINA L., TING Y.-S., DE SILVA G.M., et al. |
