Asplund, M. |
Volume |
Paper Title |
Page Number |
Authors |
96 |
Model atmospheres of cool hydrogen-deficient carbon stars |
27 |
Gustafsson, B.; Asplund, M. |
96 |
Are the declines of R Coronae Borealis stars caused by super- Eddington luminosities? |
39 |
Asplund, M.; Gustafsson, B. |
96 |
A non-LTE investigation of carbon in R Coronae Borealis stars |
57 |
Asplund, M.; Ryde, N. A. E. |
173 |
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. |
173 |
Confrontation of Stellar Surface Convection Simulations with Stellar Spectroscopy |
221 |
Asplund, M.; Nordlund, Å.; Trampedach, R. |
223 |
Effects of Convection on Line Profiles and Abundances (CD-ROM Directory: contribs/asplund) |
217 |
Asplund, M. |
223 |
Spatially Resolved Solar Lines as Diagnostics of NLTE Effects (CD-ROM Directory: contribs/kiselman) |
684 |
Kiselman, D.; Asplund, M. |
223 |
R200,000 Spectroscopic Observations of Procyon. The Surface Convection and Radial Velocity (CD-ROM Directory: contribs/allende2) |
760 |
Allende Prieto, C.; Asplund, M.; García López, R. J.; Lambert, D. L.; Nordlund, Å. |
293 |
Radiative Transfer in 3D Model Stellar Atmospheres |
197 |
Asplund, M.; Collet, R. |
293 |
Radiative Transfer with Very Few Wavelengths |
209 |
Trampedach, R.; Asplund, M. |
304 |
New Generations of Stellar Model Atmospheres (invited review) |
275 |
Asplund, M. |
336 |
The Solar Chemical Composition |
25 |
Asplund, M.; Grevesse, N.; Sauval, A.J. |
336 |
Trends and Scatter of Abundance Ratios for Metal-poor Turnoff Stars |
55 |
Nissen, P.E.; Asplund, M.; Lambert, D.L.; Primas, F.; Smith, V.V. |
374 |
Lithium Isotopic Abundances in the Early Galaxy |
119 |
Asplund, M. |
391 |
18O and the Origins of HdC and R CrB Stars |
51 |
Geballe, T.R.; Clayton, G.C.; Asplund, M.; Herwig, F.; Fryer, C. |
393 |
Signatures of Granulation in the Spectra of K-Dwarfs |
255 |
Ramirez, I.; Allende Prieto, C.; Lambert, D.L.; Asplund, M. |
396 |
Reality of Moving Groups in the Galaxy and Chemically Tagging the Galactic Disk |
59 |
De Silva, G.M.; Freeman, K.C.; Bland-Hawthorn, J.; Asplund, M. |
448 |
Effects of Scattering on the Temperature Stratification in 3D Model Atmospheres of Late-Type Stars |
819 |
Collet, R.; Hayek, W.; Asplund, M. |
448 |
Spectroscopic Microvariability Induced by Convective Motions |
1013 |
Porter, L.; Asplund, M. |
458 |
3D and NLTE Effects on Spectroscopic Parameters of Late-Type Stars |
109 |
Lind, K.; Bergemann, M.; Collet, R.; Asplund, M.; Magic, Z. |
458 |
Signatures of an Intermediate-Age Metal-Rich Bulge Population |
203 |
Bensby, T.; Feltzing, S.; Gould, A.; Johnson, J. A.; Asplund, M.; Adén, D.; Meléndez, J.; Cohen, J. G.; Thompson, I.; Lucatello, S.; Gal-Yam, A. |
458 |
Chemically Tagging Disk Fossils: the Case of the Hyades Supercluster |
215 |
De Silva, G. M.; Freeman, K. C.; Bland-Hawthorn, J.; Asplund, M. |
462 |
The New Solar Chemical Composition — from Z = 0.02 to Z = 0.013 |
41 |
Grevesse, N.; Asplund, M.; Sauval, A. J.; Scott, P. |
479 |
“Old” versus “New” Solar Chemical Composition |
481 |
Grevesse, N.; Asplund, M.; Sauval, A. J.; Scott, P. |