Ages˛: Taking Stellar Ages to the Next Power
Important! Requests to present contributed talks and requests for travel support must be submitted by June 30. Please go here.
An international astronomical symposium on the ages of stars, to be held in Elba, September 18-22, 2017.
The first "Ages of Stars" meeting was held in Baltimore, Maryland in 2008. Real progress has been made in the field since then, and Ages˛ is an opportunity to review what has been accomplished and where effort is needed. Among the subjects to be discussed are:
- Ages of clusters and age spreads, and ages of small stellar groups
- Ages of pre-main sequence stars
- Ages of the oldest stars and clusters
- Ages of low-mass stars and brown dwarfs
- Ages of evolved stars and applying them to Galactic archaeology
- The current state of stellar models
- Ages of solar-like stars from seismology and implications for gyrochronology
- Star formation histores in the Local Group
Scientists are invited to propose topics and speakers for invited talks. For additional information, please visit STScI or send an email to David Soderblom.
To register for the 2017 Ages Symposium and to find local information, please visit the University of Pisa site.
Scientific Organizing Committee
- David R. Soderblom, Chair; Space Telescope Science Institute
- Scilla Degl'Innocenti, Co-Chair; University of Pisa
- Conny Aerts, KU Leuven
- Othman Benomar, University of Tokyo
- Santi Cassisi, INAF Tergamo
- Selam de Mink, Amsterdam University
- Lynne Hillenbrand, CalTech
- Saskia Hekker, MPI Göttingen
- Daniel Huber, University of Sydney
- Rob Jeffries, Keele University
- Yveline Lebreton, Observatoire de Paris-Meudon
- Eric Mamajek, JPL
- Andrea Miglio, University of Birmingham
- Marc Pinsonneault, The Ohio State University
- Elena Sabbi, Space Telescope Science Institute
- Eline Tolstoy, Kapteyn Astronomical Institute, Groningen
What: Ages˛: Taking Stellar Ages to the Next Power
When: September 18-22, 2017
Where: Isola d'Elba, Italy
This symposium is built around six themes. Each theme has two or three conveners from the SOC who have framed key questions for the speakers to address.
Theme 1: Pre-main sequence stars and the connection to the formation and early evolution of stars and planetary systems
- L. Hillenbrand
- R. Jeffries
- E. Mamajek
- G. Somers: Testing evolutionary tracks for PMS stars including lithium depletion and radius inflation
- G. Herczeg: Effects of initial conditions and accretion on ages and star formation histories
- G. Sacco: Results for PMS stars from the Gaia/ESO and Gaia surveys
Theme 2: Solar-type and low-mass stars and the connection to exoplanets
- O. Creevey: Accuracy and systematics in asteroseismic ages for solar-type stars
- J. van Saders: Age dating using gyrochronology for solar-type stars
- K. Poppenhaeger: What age accuracies and precisions are needed for exoplanet host stars to understand planet formation and evolution?
- R. Kopparapu: What are the effects of stellar age and activity on the habitable zone?
Theme 3: Evolved stars and the connection to Galactic archaeology
- S. Hekker
- A. Miglio
- E. Tolstoy
- V. Silva Aguirre: How well can we determine ages from asteroseismology for giants?
- C. Chiappini: How old are the different components of the Galaxy and over what time-span did they form?
- A. Helmi: What are the ages of streams in galaxies and how are they determined?
- M. Tosi: What are the star formation histories of dwarf galaxies?
- C. Conroy: How ages can help understand the assembly and growth of the Milky Way
- P.-E. Tremblay: Milky Way formation history from white dwarfs
Theme 4: High- and intermediate-mass stars and the connection to clusters
- C. Aerts
- S. deMink
- E. Sabbi
- N. Bastian: Challenges for age dating young star clusters
- A. Tkachenko: The mass discrepancy in massive eclipsing binaries and its effect on ages
- C. Georgy: Ages of massive (B) stars: Effects of rotation and apparent age spreads
- F. Schneider: Ages of massive (O) stars: Effects of mergers and rejuvenated binary products
Theme 5: Ages of the oldest stars and the connection to the halo and accretion
- S. Cassisi
- S. Degl'Innocenti
- S. Hidalgo: Local Group dwarfs and the Milky Way: Implications for galaxy assembly
- A. Dotter: Abundance effects on Population II stars
- G. Piotto: Globular cluster ages: Multiple populations and age dating implications
- E. Valenti: On the age dating of old field stars
- G. Fontaine: Ages from white dwarf cooling sequences
Theme 6: Stellar models and their limitations
- Y. Lebreton
- M. Pinsonneault
- S. Randich: Constraints on models from the combined Gaia/ESO and Gaia surveys
- A. Serenelli: The current state of modeling solar-type stars
- E. Caffau: The abundance scale of stars and its effects
- J. Bailey: Opacity data for stellar models and its uncertainties
- A. Formicola: Improvements in nuclear reaction rates for stellar conditions
- On Wednesday evening, September 20th, Dr. Massimiliano Razzano (Physics Department, Pisa University and INFN, Pisa section) will be hosting a talk titled, "The dawn of gravitational wave astronomy and the multimessenger universe."
- Dr. Robert Mathieu (University of Wisconsin) will provide a special invited talk on open clusters: their promise and pitfalls.