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| NGC 884 2140 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST22:04:07 |
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 |
|---|---|---|---|---|---|---|---|---|---|
1997A&A...325..987K 
|
27 | 24 | B-type pulsators in the open cluster NGC 884 (χ Persei). | KRZESINSKI J. and PIGULSKI A. | |||||
|
2001AJ....122..248K
|
1746 | 62 | UBVI and Hα photometry of the h and χ Persei cluster. | KELLER S.C., GREBEL E.K., MILLER G.J., et al. | |||||
|
2002A&A...394..479C
|
O | 556 | 22 | CCD uvbyβ photometry of young open clusters. I. The double cluster h and χ Persei. | CAPILLA G. and FABREGAT J. | ||||
|
2002ApJ...576..880S
|
4554 | 110 | The star formation history and mass function of the double cluster h and χ Persei. | SLESNICK C.L., HILLENBRAND L.A. and MASSEY P. | |||||
|
2002PASP..114..233U
|
757 | 14 | Membership in the region of the double cluster h and χ Persei working from proper motions and positions: distance moduli and extinction in that galactic direction. | URIBE A., GARCIA-VARELA J.-A., SABOGAL-MARTINEZ B.-E., et al. | |||||
|
2005AJ....129..809S
|
775 | 60 | B star rotational velocities in h and χ Persei: a probe of initial conditions during the star formation epoch. | STROM S.E., WOLFF S.C. and DROR D.H.A. | |||||
|
2006ApJ...648..580H
|
15 | D | 517 | 132 | Stellar rotation in young clusters. I. Evolution of projected rotational velocity distributions. | HUANG W. and GIES D.R. | |||
|
2006ApJ...648..591H
|
15 | D | 482 | 63 | Stellar rotation in young clusters. II. Evolution of stellar rotation and surface helium abundance. | HUANG W. and GIES D.R. | |||
|
2008ApJ...672..558C
|
15 | D | 1 | 635 | 91 | The rise and fall of debris disks: MIPS observations of h and χ Persei and the evolution of Mid-IR emission from planet formation. | CURRIE T., KENYON S.J., BALOG Z., et al. |
