C
C. Olczak
Researcher at Max Planck Society
Publications - 4
Citations - 154
C. Olczak is an academic researcher from Max Planck Society. The author has contributed to research in topics: Star formation & Cluster (physics). The author has an hindex of 4, co-authored 4 publications receiving 142 citations. Previous affiliations of C. Olczak include Chinese Academy of Sciences & Heidelberg University.
Papers
More filters
Journal ArticleDOI
Towards a complete stellar mass function of the Hyades. I. Pan-STARRS1 optical observations of the low-mass stellar content
Bertrand Goldman,Siegfried Röser,Elena Schilbach,E. A. Magnier,C. Olczak,Th. Henning,Mario Juric,Edward F. Schlafly,Wen Ping Chen,Imants Platais,W. Burgett,K. Hodapp,J. Heasley,R. P. Kudritzki,J. S. Morgan,Paul A. Price,John L. Tonry,R. J. Wainscoat +17 more
TL;DR: In this article, the authors performed a kinematic and photometric selection using the PPMXL and Pan-STARRS1 sky surveys, to search for cluster members up to 30 pc from the cluster center.
Journal ArticleDOI
Towards a complete stellar mass function of the Hyades - I. Pan-STARRS1 optical observations of the low-mass stellar content
Bertrand Goldman,Siegfried Röser,Elena Schilbach,Eugene A. Magnier,C. Olczak,C. Olczak,C. Olczak,Th. Henning,Mario Juric,Edward F. Schlafly,Wen Ping Chen,Imants Platais,William S. Burgett,Klaus W. Hodapp,J. N. Heasley,R. P. Kudritzki,John Morgan,Paul A. Price,John L. Tonry,Richard J. Wainscoat +19 more
TL;DR: In this article, the authors performed a kinematic and photometric selection using the PPMXL and Pan-STARRS1 sky surveys, to search for cluster members up to 30 pc from the cluster center.
Journal ArticleDOI
Modes of clustered star formation
TL;DR: In this paper, the authors investigate the influence of the combination of different cluster modes, observational biases, and types of diagnostic on the results of near-neighbour searches for star and planet formation.
Journal ArticleDOI
Modes of clustered star formation
TL;DR: In this paper, near-neighbour searches are performed for model star clusters investigating the influence of the combination of different cluster modes, observational biases, and types of diagnostic and find that the cluster density profile, the relative sample sizes, limitations in observations and the choice of diagnostic method decides whether modelled modes of clustered star formation are detected.