Paper Title |
Page |
Authors |
|
| |
Fluid Dynamics in the Convective Zone |
3 |
Schatzman, E. |
Mixing in Stellar Interiors: Observational Hints |
9 |
Chiosi, C. |
Observational Evidence for Convection in Main Sequence Star Atmospheres |
21 |
Weiss, W. W.; Kupka, F. |
Critical Tests in Open Clusters: Requirements and Pitfalls |
31 |
Andersen, J.; Nordström, B. |
Eclipsing Binaries with Accurate Dimensions as a Test of Convective Core Overshooting |
41 |
Giménez, A.; Claret, A.; Ribas, I.; Jordi, C. |
Probing Convection with Helio- and Asteroseismology |
51 |
Christensen-Dalsgaard, J. |
Observational Aspects of Convection in Very Low Mass Stars and Brown Dwarfs |
67 |
Rebolo, R.; Zapatero-Osorio, M. R. |
A Ready to Use Post-MLT Recipe for General Stellar Modelling and Evolution |
77 |
Mazzitelli, I. |
Convection Simulations |
91 |
Nordlund, Å.; Stein, R. F. |
Convective Penetration in Main Sequence Stars |
103 |
Roxburgh, I. W. |
Convection in Low Mass Stars |
111 |
Baraffe, I. |
Beyond the Mixing-Length Treatment: Why and How? |
121 |
Zahn, J.-P. |
Overshooting in Stars: a New Formulation |
133 |
Canuto, V. M. |
Turbulent Convection in Pulsating Stars |
141 |
Buchler, J. R.; Yecko, P.; Kolláth, Z.; Goupil, M.-J. |
Computing Solar and Stellar Overshooting with Turbulent Convection Models. First Tests of a Fully Non-Local Model |
157 |
Kupka, F. |
Time-Dependent Turbulent Convection in Nonlinear Models of Pulsating Stars |
171 |
Feuchtinger, M. U. |
Convection, Protostellar Collapse, Deuterium Burning and Pre-Main Sequence Tracks |
181 |
Wuchterl, G. |
Convection and Giant Planet Formation |
185 |
Wuchterl, G. |
Convection and Compact Stellar Remnants in Massive Close Binaries |
189 |
Wellstein, S.; Langer, N. |
Magneto-Convection |
193 |
Stein, R. F.; Georgobiani, D.; Bercik, D. J.; Brandenburg, A.; Nordlund, Å. |
Heat Flux Transport in Low-Mass Brown Dwarfs |
197 |
Pino, D.; Mercader, I.; Net, M. |
Treatment of the Superadiabatic Convection in Low-Mass Metal-Poor Stars from Realistic Hydrodynamics Simulations: Application to Globular Clusters Isochrones |
201 |
Freytag, B.; Salaris, M.; Ludwig, H.-G. |
Convection in Metal-Poor Stars as Traced from Spectral Line Asymmetries |
205 |
Allende Prieto, C.; Asplund, M.; García López, R. J.; Gustafsson, B.; Lambert, D. L. |
Balmer Line Profiles as Stellar Atmosphere Structure Indicators |
209 |
van't Veer-Menneret, C.; Katz, D. |
Testing Convection Theories Using Balmer Line Profiles of A, F and G Stars |
213 |
Gardiner, R.; Smalley, B.; Kupka, F. |
Balmer Line Formation in Convective Stellar Atmospheres |
217 |
Steffen, M.; Ludwig, H.-G. |
Confrontation of Stellar Surface Convection Simulations with Stellar Spectroscopy |
221 |
Asplund, M.; Nordlund, Å.; Trampedach, R. |
A Calibration of the Mixing-Length for Solar-Type Stars Based on Hydrodynamical Models of Stellar Surface Convection |
225 |
Freytag, B.; Ludwig, H.-G.; Steffen, M. |
Convection and the Eclipsing Binary AI Phoenicis: How Well Can We Constrain the Mixing-Length parameter from Stellar Modelling? |
229 |
Ludwig, H.-G.; Salaries, M. |
Stellar Evolution with a Variable Mixing-Length Parameter |
233 |
Trampedach, R.; Stein, R. F.; Christensen-Dalsgaard, J.; Nordlund, Å. |
Turbulent Convection beyond Mixing-Length Models |
237 |
Houdek, G.; Gough, D. O. |
Models of Massive Stars with Turbulent Diffusion and New Mass-Loss Rates |
241 |
Salasnich, B.; Bressan, A.; Chiosi, C. |
Rotating Turbulent Compressible Convection in a Shell |
245 |
Robinson, F. J. |
The Dynamics of Rotating Convection in f-Planes |
249 |
Chan, K. L. |
Test of Convective Core Overshooting Using Evolved Eclipsing Binaries |
253 |
Ribas, I.; Jordi, C.; Giménez, A.; Claret, A.; Guinan, E. F. |
Asteroseismological Constraints on Stellar Convective Cores |
257 |
Roxburgh, I. W.; Vorontsov, S. V. |
Critical Tests of Stellar Evolution by Means of Eclipsing Binaries and Open Clusters |
261 |
Pols, O. R.; Schröder, K.-P.; Eggleton, P.; Hurley, J.; Tout, C. |
Do 0.7-1.1 Msun Eclipsing Binaries Pose a Problem for Current Stellar Evolutionary Models? |
265 |
Clausen, J. V.; Baraffe, I.; Claret, A.; Vandenberg, D. A. |
Hydrodynamical Simulations of Penetrative Convection and Generation of Internal Gravity Waves |
269 |
Kiraga, M.; Zahn, J.-P.; Stepień , K.; Jahn, K.; Rózyczka, M.; Muthsam, H. J. |
Convective Envelopes in Solar-Type Stars: What Can We Learn from their Seismic Study? |
273 |
Monteiro, M. J. P. F. G.; Christensen-Dalsgaard, J.; Thompson, M. J. |
A New Method for Calculating Gravity-Darkening Using Interior Models: Convective and Radiative Envelopes |
277 |
Claret, A. |
Coupling Between Diffusive Mixing and Nuclear Reactions: Production of Lithium in Massive AGB Stars |
281 |
Mazzitelli, I.; D'Antona, F.; Ventura, P.; Zeppieri, A. |
Lithium Abundances in AGB Stars: a Probe to Test Convective Theories and Nucleosynthesis |
285 |
Abia, C.; Isern, J. |
Carbon Burning in Intermediate Mass Stars: the Role of Convection |
289 |
García-Berro, E.; Iben, I., Jr. |
Mixing Below the Solar Convective Zone |
293 |
Brun, A. S.; Turck-Chièze, S.; Zahn, J.-P. |
The Sun as a Star: Background, Intensity and Velocity, Power Spectra and Convection |
297 |
Pallé, P. L.; Roca Cortés, T.; Jiménez, A.; GOLF team; VIRGO team |
Probing Solar Convection with p-Mode Linewidths |
301 |
Rabello-Soares, M. C.; Houdek, G.; Christensen-Dalsgaard, J. |
Low L Solar p-Mode Oscillations Parameters and Convection |
305 |
Roca Cortés, T.; Montañés, P.; Pallé, P. L.; Pérez Hernández, F.; Jiménez, A.; Régulo, C.; The GOLF Team |
On the Capability of Ground Based Networks to Precisely Estimate the Solar Background in Full Disk Helioseismology |
309 |
Fossat, E.; Kholikov, Sh.; The IRIS Team |
Granular and Intergranular Model Atmospheres from Inversion of Solar Two-Dimensional Spectroscopic Data |
313 |
Rodríguez Hidalgo, I.; Ruiz Cobo, B.; Collados, M.; del Toro Iniesta, J. C. |
On the Location of the Instability Strip |
317 |
Houdek, G.; Balmforth, N. J.; Christensen-Dalsgaard, J.; Gough, D. O. |
New Eclipsing Binaries among Late F, G, and K Type Main-Sequence Stars |
321 |
Clausen, J. V.; Helt, B. E.; Olsen, E. H. |
Constraints on the Convective Efficiency in the Outer Layers of DB White Dwarfs from the Instability Strip of the V777 HER Stars |
325 |
Wesemael, F.; Beauchamp, A.; Bergeron, P.; Fontaine, G.; Brassard, P.; Saffer, R. A.; Liebert, J. |
Convective Efficiency and the Blue Edge in ZZ Ceti Stars |
329 |
Brassard, P.; Fontaine, G. |
Evidence for Granulation in α CEN A |
333 |
Kjeldsen, H.; Bedding, T. R.; Frandsen, S.; Dall, T. H. |
AB Cas: an Eclipsing Binary System with a δ SCT Component |
337 |
Rodríguez, E.; Claret, A.; Sedano, J. L.; García, J. M.; Garrido, R. |
Photometric Effect of Rotation in δ Scuti Stars |
341 |
Pérez Hernández, F.; Claret, A.; Hernández, M. M.; Michel, E. |
Mode Identifications and Pulsation Modelling of the δ Scuti Star FG VIR |
345 |
Breger, M.; Pikall, H.; Pamyatnykh, A. A.; Garrido, R. |
Recent Photometric and Spectroscopic Results of Cepheid Variables |
349 |
Kiss, L. L.; Vinkó, J.; Balog, Z.; Alfaro, E. J.; Bakos, G. |
MONS: A Proposal for a Danish Satellite |
353 |
Kjeldsen, H.; Bedding, T. R.; Frandsen, S.; Dall, T. H.; Thomsen, B.; Christensen-Dalsgaard, J.; Clausen, J. V.; Petersen, J. O.; Andersen, M. I. |
COROT: Seismology of Stars |
357 |
Roxburgh, I. W.; The COROT Team |
What Are We Learning from the Sun? |
361 |
Roca Cortés, T. |
Which Are the Most Realistic Models to be Used? |
373 |
Demarque, P. |
Comments and Summary on the Workshop on Convection in Stellar Structure and Evolution |
383 |
Guinan, E. F. |