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Aringer, B. |
Volume |
Paper Title |
Page Number |
Authors |
259 |
Dynamical Atmospheres and Mass Loss of Pulsating AGB Stars |
534 |
Höfner, S.; Loidl, R.; Aringer, B.; Jørgensen, U. G. |
259 |
The Pulsation of M-type Miras: Multi-Epoch ISO-SWS Observations and Dynamical Models |
538 |
Aringer, B.; Jørgensen, U. G.; Kerschbaum, F.; Hron, J.; Höfner, S. |
274 |
Synthetic spectra for pulsating red giants: status, limitations and applications |
110 |
Hron, J.; Aringer, B.; Gautschy-Loidl, R.; Höfner, S.; Jørgensen, U. G. |
304 |
Abundances of C and O in Red Giant Stars |
111 |
Lebzelter, T.; Aringer, B.; Nowotny, W. |
378 |
Water Opacity in M Stars |
127 |
Lederer, M.T.; Aringer, B.; Hoefner, S.; Kerschbaum, F. |
378 |
Tracing AGB Mass Loss by (Synthetic) High-Resolution IR Spectroscopy |
325 |
Nowotny, W.; Aringer, B.; Hoefner, S. |
445 |
Photometric Modeling of Mass-losing C-type Miras |
95 |
Nowotny, W.; Aringer, B.; Höfner, S.; Lederer, M. T. |
445 |
Determination of the Stellar Parameters of C-rich Hydrostatic Stars from Spectro-Interferometric Observations |
101 |
Paladini, C.; van Belle, G. T.; Aringer, B.; Hron, J.; Reegen, P.; Lebzelter, T.; Davies, C. |
445 |
Dust in AGB Stars: Transparent or Opaque? |
315 |
Bladh, S.; Höfner, S.; Aringer, B. |
445 |
Synthetic Colors for Dynamic C-Star Models |
325 |
Eriksson, K.; Wachter, A.; Höfner, S.; Aringer, B.; Nowotny, W. |
445 |
Evolutionary Models for AGB Stars in the Magellanic Clouds |
431 |
Marigo, P.; Bressan, A.; Girardi, L.; Aringer, B.; Gullieuszik, M.; Groenewegen, M. A. T. |
448 |
Synthetic Spectra and Photometry of C-rich Hydrodynamical Model Atmospheres |
969 |
Wachter, A.; Eriksson, K.; Aringer, B.; Höfner, S.; Nowotny, W. |
497 |
A New Library of Synthetic Spectra and Photometry for Evolved
C Stars |
111 |
Eriksson, K.; Nowotny, W.; Höfner, S.; Aringer, B. |
497 |
Carbon Stars from the X-shooter Spectral Library |
113 |
Gonneau, A.; Lançon, A.; Trager, S.; Aringer, B.; Nowotny, W.; Chen, Y.-P.; Peletier, R. |
497 |
The Close Environment of the C-star TX Psc as Seen with CRIRES Spectro-Astrometry |
121 |
Hron, J.; Lebzelter, T.; Paladini, C.; Uttenthaler, S.; Aringer, B.; Wiedemann, G. |
497 |
Into the Modelling of RU Vir |
137 |
Rau, G.; Hron, J.; Paladini, C.; Eriksson, K.; Aringer, B.; Groenewegen, M. A. T.; Mečina, M. |
497 |
Winds of Binary AGB Stars as Observed by Herschel |
181 |
Mayer, A.; Jorissen, A.; Kerschbaum, F.; Ottensamer, R.; Mečina, M.; Paladini, C.; Cox, N. L. J.; Nowotny, W.; Aringer, B.; Pourbaix, D.; Mohamed, S.; Siopis, C.; Groenewegen, M. A. T. |
497 |
The Challenges of Abundance Analysis for Long–Period Variables |
283 |
Lebzelter, T.; Nowotny, W.; Hinkle, K. H.; Höfner, S.; Aringer, B.; Heiter, U. |
497 |
Fluorine Abundances of AGB Stars in Stellar Clusters |
305 |
Hren, A.; Lebzelter, T.; Aringer, B.; Hinkle, K. H.; Nowotny, W. |
497 |
Exploring Mass-Loss in M-type AGB Stars |
345 |
Bladh, S.; Höfner, S.; Aringer, B.; Eriksson, K. |
497 |
How Important Are Metal-Poor AGB Stars As Cosmic Dust Producers? |
385 |
Mattsson, L.; Aringer, B.; Andersen, A. C. |
497 |
Dust in Stellar Winds: A Micro- and Macroscopic View |
395 |
Mečina, M.; Groenewegen, M. A. T.; Kerschbaum, F.; Aringer, B.; Nowotny, W.; Ottensamer, R.; Mayer, A.; Luntzer, A. |
497 |
Modelling the AGB Dust Evolution |
397 |
Nowotny, W.; Gail, H.-P.; Posch, Th.; Aringer, B. |
497 |
Constraining Mass Loss and Lifetimes of Low Mass, Low
Metallicity AGB Stars |
423 |
Rosenfield, P.; Marigo, P.; Girardi, L.; Dalcanton, J. J.; Bressan, A.; Gullieuszik, M.; Weisz, D. R.; Williams, B. F.; Dolphin, A.; Aringer, B. |
497 |
Where is the Metallicity Ceiling to Form Carbon Stars? – A Scarcity of Carbon Stars in the Inner Disk of M31 |
479 |
Boyer, M. L.; Girardi, L.; Marigo, P.; Williams, B. F.; Aringer, B.; Nowotny, W.; Rosenfield, P.; Dorman, C. E.; Guhathakurta, P.; Dalcanton, J. J.; Melbourne, J. L.; Olsen, K. A. G.; Weisz, D. R. |
514 |
Modelling TP-AGB Stars in M31 with PHAT Data |
57 |
Chen, Y.; Marigo, P.; Girardi, L.; Pastorelli, G.; Williams, B. F.; Rosenfield, P.; Dalcanton, J. J.; Aringer, B.; Trabucchi, M |
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