List of abstracts received for SCYON
List of abstracts by order of arrival date
Issue No 11, October 31 2002
Sections
- Star forming region
- Embedded clusters
- Galactic open clusers
- Galactic globular clusters
- Galactic center clusters
- SMC clusters
- LMC clusters
- Extragalactic clusters
- Cluster formation
- Dynamical evolution - simulations
- Miscellanous
A. Star Forming Regions
B. Embedded Clusters
C. Galactic Open Clusters
N.V. Kharchenko, L.K. Pakulyak & A.E. Piskunov (October 25, 2002)
- Subsystem of open clusters in post Hipparcos epoch. Structure parameters and proper motions
E. Flaccomio, G. Micela, S. Sciortino (September 21, 2002)
- Observational clues for a role of circumstellar accretion in PMS X-ray activity
J. Bouvier, E. Moraux, J.R. Stauffer, D. Barrado y Navascués & J.-C. Cuillandre (September 6, 2002)
- The Lower Mass Function of Young Open Clusters
R.K.S. Yadav & Ram Sagar (August 28, 2002)
- A deep UBVRI CCD photometric study of the open clusters Tr 1 and Be 11
D. Galactic Globular Clusters
Holger Baumgardt, Piet Hut, Junichiro Makino, Steve McMillan, Simon Portegies Zwart (October 29, 2002)
- On the central structure of M15
Robert P. Kraft, Inese I. Ivans (October 29, 2002)
- A Globular Cluster Metallicity Scale Based on the Abundance of FeII
Mirek Giersz and Douglas C. Heggie (October 22, 2002)
- A Simple Dynamical Model for Omega Cen
E. Galactic Center Clusters
F. SMC Clusters
G. LMC Clusters
H. Extragalactic Clusters
Cristiano Da Rocha, Claudia Mendes de Oliveira, Michael Bolte, Bodo L. Ziegler, Thomas H. Puzia (October 25, 2002)
- Globular Clusters in Compact Groups
S.S. Larsen, J.P. Brodie, A. Sarajedini, J.P. Huchra (August 26, 2002)
- Structural Parameters and Dynamical Masses for Globular Clusters in M33
I. Cluster formation
C.M. Boily, P. Kroupa (October 30, 2002)
- The impact of mass loss on star cluster formation. I. Analytic results
B.G. Elmegreen, Mohsen Shadmehri (October 18, 2002)
- Constraints on star formation from the close packing of protostars in clusters
J. Dynamical Evolution - Simulations
K. Miscellanous