Presentation is loading. Please wait.

Presentation is loading. Please wait.

Confronting predictions of stellar evolution theory gregory feiden (uppsala) andrew mann (texas at austin) eric gaidos (hawaii) tabetha boyajian (yale)

Published byAubrey Barnett Modified over 8 years ago

Similar presentations

Presentation on theme: "Confronting predictions of stellar evolution theory gregory feiden (uppsala) andrew mann (texas at austin) eric gaidos (hawaii) tabetha boyajian (yale)"— Presentation transcript:

1 confronting predictions of stellar evolution theory gregory feiden (uppsala) andrew mann (texas at austin) eric gaidos (hawaii) tabetha boyajian (yale) the case of single field stars @GFeiden

2 knowing your dwarf 05 Jan 2015AAS 225 Feiden & Chaboyer (2012, ApJ, 757, 42)Boyajian et al. (2012, ApJ, 757, 112)

3 parameter inference 05 Jan 2015AAS 225 Gl 411

4 model reliability 05 Jan 2015AAS 225

5 origins 05 Jan 2015AAS 225

6 origins 05 Jan 2015AAS 225

7 empirically determining dwarf properties and model comparisons 05 Jan 2015AAS 225 see talk by andrew mann 130.01 full paper on the arXiv this week

Download ppt "Confronting predictions of stellar evolution theory gregory feiden (uppsala) andrew mann (texas at austin) eric gaidos (hawaii) tabetha boyajian (yale)"

Similar presentations

Late gas accretion onto primordial mini-halos a model for pre-reionization dwarfs and extragalactic compact High-Velocity Clouds Massimo Ricotti (U of.

Late gas accretion onto primordial mini-halos a model for pre-reionization dwarfs and extragalactic compact High-Velocity Clouds Massimo Ricotti (U of.
1 MSci Astrophysics 210PHY412 Stellar structure and evolution Dr. Stephen Smartt (Room S039) Department of Physics and Astronomy Online.

1 MSci Astrophysics 210PHY412 Stellar structure and evolution Dr. Stephen Smartt (Room S039) Department of Physics and Astronomy Online.
Small is Beautiful: Cataclysmic Variables from the SDSS John Southworth Boris Gänsicke Tom Marsh + many others.

Small is Beautiful: Cataclysmic Variables from the SDSS John Southworth Boris Gänsicke Tom Marsh + many others.
Including Magnetic Effects in 1-D Stellar Models Greg Feiden & Brian Chaboyer (Dartmouth) Three color EUV image of the Sun. White lines show a model of.

Including Magnetic Effects in 1-D Stellar Models Greg Feiden & Brian Chaboyer (Dartmouth) Three color EUV image of the Sun. White lines show a model of.
Improving mass and age estimates of unresolved stellar clusters Margaret Hanson & Bogdan Popescu Department of Physics.

Improving mass and age estimates of unresolved stellar clusters Margaret Hanson & Bogdan Popescu Department of Physics.
The Group of Bootis Stars Dr. Ernst Paunzen Institute for Astronomy University of Vienna.

The Group of Bootis Stars Dr. Ernst Paunzen Institute for Astronomy University of Vienna.
The Distribution of DM in Galaxies Paolo Salucci (SISSA) TeVPa Paris,2010.

The Distribution of DM in Galaxies Paolo Salucci (SISSA) TeVPa Paris,2010.
Exoplanet- Asteroseismology Synergies Bill Chaplin, School of Physics & Astronomy University of Birmingham, UK EAHS2012, Oxford, 2012 March 15.

Exoplanet- Asteroseismology Synergies Bill Chaplin, School of Physics & Astronomy University of Birmingham, UK EAHS2012, Oxford, 2012 March 15.
Eric Y. Hsiao University of Victoria.  less dust extinction  low redshift  standard candles in JHK bands  independent measure of Hubble constant 

Eric Y. Hsiao University of Victoria.  less dust extinction  low redshift  standard candles in JHK bands  independent measure of Hubble constant 
SOLUTION 1: ECLIPSING BINARIES IN OPEN CLUSTERS The study of eclipsing binaries in open clusters allows strong constraints to be placed on theoretical.

SOLUTION 1: ECLIPSING BINARIES IN OPEN CLUSTERS The study of eclipsing binaries in open clusters allows strong constraints to be placed on theoretical.
Venice – Gregory RudnickMarch 2006 The Mean SED and Stellar Mass Density at z

Venice – Gregory RudnickMarch 2006 The Mean SED and Stellar Mass Density at z
Q. Daniel Wang and Cornelia Lang (U. of Massachusetts) Eric Gotthelf (Columbia U.) Chandra X-ray Survey of the Galactic Center: On the Nature of the X-ray.

Q. Daniel Wang and Cornelia Lang (U. of Massachusetts) Eric Gotthelf (Columbia U.) Chandra X-ray Survey of the Galactic Center: On the Nature of the X-ray.
Multiple, Coeval and Hubble-like bipolar outflows Romano L.M. Corradi Isaac Newton Group of Telescopes La Palma, Spain.

Multiple, Coeval and Hubble-like bipolar outflows Romano L.M. Corradi Isaac Newton Group of Telescopes La Palma, Spain.
General Principles for References Use the most original source possible. Use the most up-to-date and reliable source available. Your paper is only as good.

General Principles for References Use the most original source possible. Use the most up-to-date and reliable source available. Your paper is only as good.
PhyloSub Jiao et. al. BMC Bioinformatics 2014, 15:35.

PhyloSub Jiao et. al. BMC Bioinformatics 2014, 15:35.
Advanced Methods for Studying Astronomical Populations: Inferring Distributions and Evolution of Derived (not Measured!) Quantities Brandon C. Kelly (CfA,

Advanced Methods for Studying Astronomical Populations: Inferring Distributions and Evolution of Derived (not Measured!) Quantities Brandon C. Kelly (CfA,
Extrasolar Planets Z:\exo\presentations\EGS2001_exo.ppt, 24.08.2015 10:54AM, 1 Tidal interactions of close-in extrasolar planets with their host stars.

Extrasolar Planets Z:\exo\presentations\EGS2001_exo.ppt, :54AM, 1 Tidal interactions of close-in extrasolar planets with their host stars.
References: Sozzetti, A., et al. 2007, ApJ, 664, 1190 Mandushev, G., et al. 2007, ApJ, 667, L195 Sozzetti, A., et al. 2007a, ApJ, in preparation Sozzetti,

References: Sozzetti, A., et al. 2007, ApJ, 664, 1190 Mandushev, G., et al. 2007, ApJ, 667, L195 Sozzetti, A., et al. 2007a, ApJ, in preparation Sozzetti,
A New Technique to Measure ΔY/ΔZ A. A. R. Valcarce (UFRN) Main collaborators: J. R. de Medeiros (UFRN)M. Catelan (PUC) XXXVII SAB meeting Águas de Lindóia,

A New Technique to Measure ΔY/ΔZ A. A. R. Valcarce (UFRN) Main collaborators: J. R. de Medeiros (UFRN)M. Catelan (PUC) XXXVII SAB meeting Águas de Lindóia,
I N T R O D U C T I O N The mechanism of galaxy formation involves the cooling and condensation of baryons inside the gravitational potential well provided.

I N T R O D U C T I O N The mechanism of galaxy formation involves the cooling and condensation of baryons inside the gravitational potential well provided.

Similar presentations

Ads by Google