List of abstracts received for SCYON

List of abstracts by order of arrival date

Issue No 56, September 12 2012

Sections

  1. Star forming region
  2. Embedded clusters
  3. Galactic open clusters
  4. Galactic globular clusters
  5. Galactic center clusters
  6. SMC clusters
  7. LMC clusters
  8. Extragalactic clusters
  9. Cluster formation
  10. Dynamical evolution - simulations
  11. Miscellanous


A. Star Forming Regions


B. Embedded Clusters


C. Galactic Open Clusters

N.V. Kharchenko, A.E. Piskunov, E. Schilbach, S. Röser, and R.-D. Scholz  (September 07 2012)
Global survey of star clusters in the Milky Way I. The pipeline and fundamental parameters in the second quadrant

I. Negueruela, A. Marco, C. Gonzélez-Fernández, F. Jiménez-Esteban, J.S. Clark, M. Garcia, and E. Solano  (September 06 2012)
Red supergiants around the obscured open cluster Stephenson 2

L. Prisinzano, G. Micela, S. Sciortino, L. Affer and F. Damiani  (September 05 2012)
Spectral classification and HR diagram of pre-main sequence stars in NGC6530

Ting, Yuan-Sen, De Silva, Gayandhi, Freeman, Ken Parker, Stacey-Jo  (September 04 2012)
High resolution elemental abundances analysis of the open cluster IC 4756


D. Galactic Globular Clusters

D. Majaess, D.G. Turner, W. Gieren, and D.J. Lane  (June 14 2012)
The Impact of Contaminated RR Lyrae/Globular Cluster Photometry on the Distance Scale


E. Galactic Center Clusters


F. SMC Clusters


G. LMC Clusters

V. Henault-Brunet, C.J. Evans, H. Sana, M. Gieles, N. Bastian, J. Maiz Apellaniz, N. Markova, W.D. Taylor, E. Bressert, P.A. Crowther, and J. Th. van Loon  (August 10 2012)
The VLT-FLAMES Tarantula Survey. VII. A low velocity dispersion for the young massive cluster R136

V. Henault-Brunet, M. Gieles, C.J. Evans, H. Sana, N. Bastian, J. Maiz Apellaniz, W.D. Taylor, N. Markova, E. Bressert, A. de Koter, and J. Th. van Loon  (August 09 2012)
The VLT-FLAMES Tarantula Survey. VI. Evidence for rotation of the young massive cluster R136


H. Extragalactic Clusters


I. Cluster formation


J. Dynamical Evolution - Simulations

Stefan Umbreit, John M. Fregeau, Sourav Chatterjee, Frederic A. Rasio  (September 10 2012)
Monte Carlo Simulations of Globular Cluster Evolution. VI. The Influence of an Intermediate-mass Black Hole

Sanghamitra Goswami, Stefan Umbreit, Matt Bierbaum, and Frederic A. Rasio  (September 10 2012)
Formation of Massive Black Holes in Dense Star Clusters. II. Initial Mass Function and Primordial Mass Segregation

Bharath Pattabiraman, Stefan Umbreit, Wei-King Liao, Alok Choudhary, Vassiliki Kalogera, Gokhan Memik, and Frederic A. Rasio  (September 10 2012)
A Parallel Monte Carlo Code for Simulating Collisional N-body Systems

Stefan Umbreit and Frederic A. Rasio  (September 10 2012)
Constraining Intermediate-Mass Black Holes in Globular Clusters

B. Pattabiraman, S. Umbreit, W. Liao, F. Rasio, V. Kalogera, and A. Choudhary  (September 10 2012)
GPU-Accelerated Monte Carlo Simulations of Dense Stellar Systems

Sambaran Banerjee, Pavel Kroupa, and Seungkyung Oh  (September 08 2012)
The emergence of super-canonical stars in R136-type star-burst clusters

H. Baumgardt, G. Parmentier, P. Anders, and E. Grebel  (September 08 2012)
The star cluster formation history of the LMC

Geneviéve Parmentier and Holger Baumgardt  (September 07 2012)
The mass function and dynamical mass of young star clusters: Why their initial crossing-time matters crucially

S. Pfalzner, T. Kaczmarek, C. Olczak  (September 07 2012)
Modes of clustered star formation

Sourav Chatterjee, Stefan Umbreit, John M. Fregeau, and Frederic A. Rasio  (September 06 2012)
Understanding the Dynamical State of Globular Clusters: Core-Collapsed vs Non Core-Collapsed

David Merritt and Eugene Vasiliev  (September 04 2012)
Spin Evolution of Supermassive Black Holes and Galactic Nuclei

Mark Gieles, Nick Moeckel, and Cathie J. Clarke  (July 10 2012)
Do all stars in the solar neighbourhood form in clusters? A cautionary note on the use of the distribution of surface densities

M.S. Oey  (July 02 2012)
The Salpeter Slope of the IMF Explained


K. Miscellanous