IoA Stellar Pops
The Institute of Astronomy Stellar Populations group meetings and talks.
Contact: Laura Watkins ; Alis Deason
0 upcoming talks View 84 archived talks
Please see above for contact details for this list.
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IoA Stellar Pops
Further detail
The Institute of Astronomy Stellar Populations group meetings and talks. If you have a question about this list, please contact: Laura Watkins; Alis Deason. If you have a question about a specific talk, click on that talk to find its organiser. 0 upcoming talks and 84 talks in the archive. Galaxia: A Code to Generate a Synthetic Survey of the Milky Way
Flattening, Anisotropy and the Dark Halo
Multiple Populations in Dwarf Spheroidals: Theoretical Perspective
Pre-reionization Fossils, Ghost Halos and the Missing Massive Satellites
Multiple Populations in Dwarf Spheroidals: Observational Perspective
Microlensing: Marching Toward a Complete Census of Cold Exoplanet Population
Stellar Archaeology: New Science with Old stars
Two Work in Progress Talks (30 minutes each)
Observational and Theoretical Adventures in Phase Space
The life cycle of star clusters in a tidal field
A novel method of exploring the star-forming history of galaxies using Red Supergiants
New Insights into The Sagittarius Stream
Early-Type Galaxies: A Miscellany of Topics
Binary Stars as Probes of Dark Substructure
RR Lyrae variables and other distance indicators in the Local Group
Velocity Dispersions and Dark Matter Limits in Globular Clusters
The Modelling of the Dwarf Spheroidals
Tidal Stripping, Compact Ellipticals, and Ultracompact Dwarf Galaxies
Globular clusters are not small galaxies
Bootes dwarf spheroidal kinematics: Techniques and first results from high precision multi-epoch radial velocity measurements
Science Alerts with GAIA : Update and Future Developments
Weakening dark-matter cusps by clumpy baryonic infall
Binary Stars as Probes of Dark Substructure
Dynamics of tidal fields and early evolution of star clusters in galaxy mergers
Testing LambdaCDM with Dwarf Spheroidals
The Stellar Halos of the Milky Way as seen by SDSS. The Expanded View
The Local Group Dwarf Spheroidals: The Variable Star View.
Photometric Studies of the Ultra-Faint Dwarfs
Evidence for Rotating Milky Way Halo Stellar Populations
Properties of the central velocity dispersion and half-light radius in dwarf spheroidals
The Star Formation Histories of M31 Halo Substructures
The Uncertainty in the Milky Way's Parameters
Exploring the Sagittarius luminosity profile using simulations
Self-similar evolution of (globular) star clusters: comparing structural parameters of Milky Way globular clusters to the theory
An Introduction to the Vista Hemisphere Survey
Galaxy Formation and Evolution in the Next Decade
A Pessimist's Guide to Indirect Dark Matter Detection
Radial velocities and proper motions: doing better
Looking at the Canes Venatici I and Carina dSphs through Monte Carlo Techniques
The "why and how" of the new Hipparcos reduction & some first science results
Star formation and stellar populations in the Local Volume
Intergalactic Globular Clusters in the Coma Cluster
Towards Understanding the Sagittarius' Orbit
The Milky Way halo: Modeling of the satellites and thin stellar streams
Real-time photometric monitoring with Gaia Science Alerts
Statistics of Milky Way-type Satellites and their Substructure
2MASS vs SDSS in the Sagittarius Stream
Understanding the Sagittarius dwarf galaxy
Identification of substructure in phase-space using orbital frequencies
Faint substructure revealed by RR Lyraes in Stripe 82
A Pilot Survey of Stellar Tidal Streams in Nearby Spiral Galaxies
Photometric constraints on white dwarfs and the identification of extreme objects
Segue 1 - The most dark matter dominated galaxy or a disrupting star cluster
Signatures of stellar mass stripping in Local Group dSphs
An Introduction to the Stellar Pops Group
The Universality of the Globular Cluster Mass Function - Can Dynamical Evolution be Ruled Out?
Analysis of subdwarfs in Stripe 82: Investigation into kinematic substucture.
The quantification of bar strength in galaxies.
A robust statistical estimation of the basic parameters of single stellar populations.
Luminosity function of MW satellites: Observational constraints on the "missing satellite" problem.
New results on the Sagittarius Stream in Stripe 82.
Please see above for contact details for this list. |
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