Articles found in WEBDA
Criteria :
- Year interval : 2004 to 2014
- Keyword: Be59
Bibliography 2004
No article foundBibliography 2005
Kharchenko N.V., Piskunov A.E., Röser S., Schilbach E., Scholz R.-D.
(2005) Astron. Astrophys. 438, 1163
Astrophysical parameters of galactic open clusters
2005A&A...438.1163K
Bibliography 2006
No article foundBibliography 2007
No article foundBibliography 2008
No article foundBibliography 2009
Kharchenko N.V., Berczik P., Petrov M.I., Piskunov A.E., Röser S., Schilbach E., Scholz R.-D.
(2009) Astron. Astrophys. 495, 807
Shape parameters of Galactic open clusters
2009A&A...495..807K
Kharchenko N.V., Piskunov A.E., Röser S., Schilbach E., Scholz R.-D., Zinnecker H.
(2009) Astron. Astrophys. 504, 681
Integrated BVJHKs parameters and luminosity functions of 650 Galactic open clusters
2009A&A...504..681K
Bibliography 2010
No article foundBibliography 2011
Piskunov A.E., Kharchenko N.V., Schilbach E., Röser S., Scholz R.-D., Zinnecker H.
(2011) Astron. Astrophys. 525, A122
The evolution of luminosity, colour, and the mass-to-luminosity ratio of Galactic open clusters. Comparison of discrete vs. continuous IMF models
2011A&A...525A.122P
Lata S., Pandey A.K., Maheswar G., Mondal S., Kumar B.
(2011) Mon. Not. R. Astron. Soc. 418, 1346
Photometric search for variable stars in the young open cluster Berkeley 59
2011MNRAS.418.1346L
Bibliography 2012
Koenig X.P., Leisawitz D.T., Benford D.J., Rebull L.M., Padgett D.L., Assef R.J.
(2012) Astrophys. J. 744, 130
Wide-field Infrared Survey Explorer Observations of the Evolution of Massive Star-forming Regions
2012ApJ...744..130K
Eswaraiah C., Pandey A.K., Maheswar G., Chen W.P., Ojha D.K., Chandola H.C.
(2012) Mon. Not. R. Astron. Soc. 419, 2587
Broad-band optical polarimetric studies towards the Galactic young star cluster Berkeley 59
2012MNRAS.419.2587E
Bibliography 2013
No article foundBibliography 2014
Ozeren F.F., Arslan O., Kucuk I., Oralhan I.A.
(2014) New Astronomy 32, 36
Analytical studies of NGC 2571, NGC 6802, Koposov 53 and Be 89
2014NewA...32...36O
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