rr lyraes bi-qing for chris sneden (ut) george preston (carnegie observatory)
TRANSCRIPT
RR LyraesRR Lyraes
Bi-Qing ForBi-Qing For
Chris Sneden (UT) Chris Sneden (UT)
George Preston (Carnegie Observatory)George Preston (Carnegie Observatory)
What are RR Lyrae stars?What are RR Lyrae stars?
APOD 23 Feb 2001
What happens when stars cross What happens when stars cross the instability strip? the instability strip?
They pulsate like a jello!
Scientific Computing in the School of Physics at the University of Sydney
RR LyraesRR Lyraes
Max radius
Typical time scale = 0.57 day
Different types of RR LyraesDifferent types of RR Lyraes
What drives stellar pulsations?What drives stellar pulsations?
• Kappa-mechanism (RR Lyrs)– “steam engine”
Absorb heat
Restore the balance inside the star
Release heat / cool off
Contract Expand
Why RR Lyraes are interesting? Why RR Lyraes are interesting?
• Most of RR Lyraes have – stable pulsation – stable pulsational period– high luminosity
• Easy to be identified at large distances
• Standard candles for distance scale
• Tracers for Studying Galactic structure
Distance scale to Globular ClustersDistance scale to Globular Clusters
https://www.cfa.harvard.edu/~jhartman/M3_movies.html
M 3
Duffau et al. (2006)
Tracers for studying Galactic structureTracers for studying Galactic structure
Special: Blazhko effectSpecial: Blazhko effect
Sergey Blazhko
created by D. Welch based on MACHO project data, Alcock et al. 2000
What am I studying?What am I studying?• Chemical compositions throughout the
pulsational cycle.
• Line profile variation
• Where do we get the spectra?
George Preston
LCO
Du Pont 100 inch
What do we learn?What do we learn?
Line profile variationLine profile variation
Chemical CompositionsChemical Compositions
Current MissionsCurrent Missions
CoRoT - COnvection, ROtation & Transits planétaires
Kepler Space Telescope
Many new RR Lyrs have been discovered
New properties have been found in the lightcurves of RR Lyrs