The Future of Cool-Star Astrophysics


July 30th - August 3rd, 2001, Boulder, Colorado


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Thursday 2nd August 2001

Session V -- Physical Processes I - General Introduction [Chair Juergen Schmitt]
Karel Schrijver (Lockheed Martin - Palo Alto) -- Modeling Atmospheric Activity of Cool Stars (Invited Review) 240
    Ness: Influence of UV Radiation Fields on Density Diagnostics with He-like Triplets265
    Reiners: Detection of Differential Rotation in Psi Cap with Profile Analysis 275
    Morossi: Far-UV Continuum as a Diagnostic for Temperature Structure in the Atmospheres of G-type Stars 285
Physical Processes II - Coronal Structure and Processes
    Audard: A Study of the Coronal Plasma in RS CVn Binary Systems 293
    Osten: Chandra, EUVE, and VLA Observations of the Active Binary System Sigma^2 CrB---
    Guedel: A Systematic Spectroscopic X-Ray Study of Stellar Coronae with XMM-Newton: Early Results303
Physical Processes III - Detailed Modelling of Atmospheric Phenomena
    Raassen: Temperatures, Densities, Abundances of Alpha Cen and Procyon 313
    McMurry: Dynamic Modelling of the Outer Atmosphere of Alpha Tau323
    Lobel: Chromospheric Dynamics of Betelgeuse from STIS Spectra 329
Physical Processes IV - Back to the Surface, and out to the Interplanetary Medium
    Gray: Giant Convection Cells, Where Are You? 344
    Wood: Mass Loss of Solar-Like Stars from H I Ly-alpha Absorption 349
[Monday] [Tuesday] [Wednesday] [Thursday] [Friday]