Star Clusters in the Era of Large Surveys Proceedings of Symposium 5 of JENAM 2010 /
The symposium “Star Clusters in the Era of Large Surveys” was held in Lisbon on Sep 9-10 during the JENAM 2010. It served as a platform for discussing what and how recent, on-going and planned large-area ground-based and space-based surveys can contribute to producing a major leap in this research f...
| Συγγραφή απο Οργανισμό/Αρχή: | |
|---|---|
| Άλλοι συγγραφείς: | , |
| Μορφή: | Ηλεκτρονική πηγή Ηλ. βιβλίο |
| Γλώσσα: | English |
| Έκδοση: |
Berlin, Heidelberg :
Springer Berlin Heidelberg : Imprint: Springer,
2012.
|
| Σειρά: | Astrophysics and Space Science Proceedings,
|
| Θέματα: | |
| Διαθέσιμο Online: | Full Text via HEAL-Link |
Πίνακας περιεχομένων:
- Part I Recent, on-going and planned surveys. Cluster searches. Technical challenges
- Optical digital Galactic Plane surveys and star-cluster science
- Census of Milky Way Star Clusters from Infrared Surveys
- Time-resolved surveys of stellar clusters
- SDSS-III/APOGEE: Detailed Abundances of Galactic Star Clusters
- Processing Data from Large Infrared Surveys
- Properties of Star Clusters Found and Investigated by Data from Large Surveys
- Developments of the open cluster database WEBDA
- Inferring stellar properties using colours, parallaxes and an HRD prior
- AstrOmatic software in the era of large stellar photometric surveys
- Cluster parameter determinations for large datasets
- Open clusters science in the Virtual Observatory era
- GALExtin: A VO-Service for estimating Galactic interstellar extinction
- YSO clusters on galactic infrared loops
- VVV Search for New Young Clusters Towards the Star Forming Regions in our Galaxy. First Results
- New MilkyWay star cluster candidates from DSS and 2MASS
- VVV study of the young Milky Way star clusters: Mercer 35, 69 and 70
- Part II Star formation & evolution. The MilkyWay and beyond
- Optical surveys of young open clusters
- Probing the low-mass end of the IMF in star-forming regions: a WIRCam/CFHT Survey
- Dynamics in the embedded phase: accretion, collisions, contraction
- Unraveling the initial conditions of star formation in Serpens North
- Do All Stars in the Solar Neighbourhood Form in Clusters?
- Uncertainties in the Age Scale for Young Open Clusters and Moving Groups
- Are there age spreads in star forming regions?
- The relevance of X-ray surveys for the study of the properties of young open clusters
- Chandra observations of Cygnus OB2
- Young massive stellar clusters in the Milky Way: the Cl1813-178 and GLIMPSE 9 clusters
- Multiple populations in Globular Clusters: The role of AGB and super-AGB stars
- Chemical properties of the open cluster population
- Deep and extended multiband photometry of the Galactic globular cluster M71
- Chromospheric activity and Lithium abundance in NGC2516
- A deep photometric survey of the double cluster h & c Per
- A detailed spectroscopic analysis of the open cluster NGC 5460
- A kinematic study of open clusters: implications for origin
- The Luminosity Function of Globular Clusters Used as a Distance Indicator
- Chemical properties of the Hipparcos red clump
- Chemical composition of a kinematically identified stellar group in the MilkyWay
- Star Disk Interaction in T Tauri Stars: Analysis of the MgII Lines
- Indication of Mass Segregation in LMC Star Clusters
- Carbon and nitrogen as tracers of stellar evolution in red clump stars of open clusters
- Observations of the IMF in clusters
- Dynamical evolution of rotating globular clusters with embedded black holes
- Stellar populations in the super star clusters NGC 3603 and 30 Doradus
- Dynamical Expansion of Star Clusters
- The Metallicity Gradient in the Galactic Disk Revealed by Cepheids and Open Clusters
- Spitzer’s view of NGC2264’s circumstellar disk population
- Super star clusters in IR-luminous interacting galaxies: the NIR luminosity function
- Populations of Variable Stars in Open Clusters
- Tracing the structure of the Perseus Arm with IPHAS
- Setting up the T35 telescope at Sierra Nevada Observatory for detecting variable stars in open clusters
- The substellar population of the s Orionis cluster.
