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Symposium - International Astronomical Union, The Carbon Star Phenomenon

Volume 177 - 2000

This volume was published under a former title. See this journal's title history.

Contents

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Abstracts of Posters

The Backwarming Effect and Carbon Stars
Dimitri N. Doikov, Ekaterina M. Doikova
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25 May 2016, p. 529
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Proposal for a Photometric System for the Classification of Carbon Stars
Uldis Dzervitis
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25 May 2016, p. 530
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Carbon to Oxygen Abundance Ratios in the Atmospheres of Carbon Stars of the Orion and Perseus Galactic Arms
I. Eglitis, M. Eglite
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25 May 2016, p. 531
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Condensation of SiC in Circumstellar Dust Shells of C-Rich Red Giants
Andreas Gauger, John J. Ready, Erwin Sedlmayr
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25 May 2016, p. 532
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New Results from the Modeling of the Shell around IRC + 10216
M. A. T. Groenewegen
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25 May 2016, p. 533
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JHK Photometry of AGB Stars in the SMC
M. A. T. Groenewegen, J. A. D. L. Blommaert
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25 May 2016, p. 534
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Frequency Sampling for Radiative Transfer Calculations in Cool Stars
Christiane Helling, Uffe Gråe Jørgensen
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25 May 2016, p. 535
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Macro-Molecules in Model Atmospheres
Christiane Helling, Uffe Gråe Jørgensen, Bertrand Plez, Hollis R. Johnson
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25 May 2016, p. 536
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Molecular Hydrogen in the Circumstellar Shells of Carbon Stars
Kenneth Hinkle, John Keady
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25 May 2016, p. 537
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Atmospheric Dynamics and Dust-Driven Winds of Carbon Stars
Susanne Höfner, Ernst A. Dorfi
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25 May 2016, p. 538
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The Shape of Silicate Features in Semiregular and Mira Variables
Josef Hron, Bernhard Aringer, Franz Kerschbaum
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25 May 2016, p. 539
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FG Sge as a New–Born Carbon Star
Takashi Iijima
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25 May 2016, p. 540
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Experimental Gas-Phase Spectroscopy of Carbon Molecular Structures and Diffuse Interstellar Bands
J. Janča, M. Plonka, M. Šolc, M. Vetešník
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25 May 2016, p. 541
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The Population of Red Giant Stars in Globular Clusters of the Fornax Dwarf Galaxy
Uffe Gråe Jørgensen, Raul Jimenez
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25 May 2016, p. 542
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Synthetic JHK Colors for M Dwarfs, M Giants, and Carbon Stars
Uffe Gråe Jørgensen, Robert F. Wing
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25 May 2016, p. 543
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Near-Infrared Spectroscopy of High Galactic Latitude Carbon Stars – They Might Be Giants?
Richard R. Joyce
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25 May 2016, p. 544
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A Simulation for a Carbon Star
Gülçin Kandemir, Cem Güçlü
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25 May 2016, p. 545
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On the Nature of Irregular Variables of Type Lb
Franz Kerschbaum, Peter Habison, Josef Hron
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25 May 2016, p. 546
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Comparison of C-Rich Mira, Semiregular, and Irregular Variables
Franz Kerschbaum, Peter Habison, Rita Loidl, Hans Olofsson, Josef Hron
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25 May 2016, p. 547
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The Chemical Composition of the Halo Mira V CrB
Tônu Kipper, Uffe G. Jørgensen
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25 May 2016, p. 548
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Proceedings of the International Astronomical Union

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Symposium - International Astronomical Union, The Carbon Star Phenomenon

Abstracts of Posters

The Backwarming Effect and Carbon Stars

Proposal for a Photometric System for the Classification of Carbon Stars

Carbon to Oxygen Abundance Ratios in the Atmospheres of Carbon Stars of the Orion and Perseus Galactic Arms

Condensation of SiC in Circumstellar Dust Shells of C-Rich Red Giants

New Results from the Modeling of the Shell around IRC + 10216

JHK Photometry of AGB Stars in the SMC

Frequency Sampling for Radiative Transfer Calculations in Cool Stars

Macro-Molecules in Model Atmospheres

Molecular Hydrogen in the Circumstellar Shells of Carbon Stars

Atmospheric Dynamics and Dust-Driven Winds of Carbon Stars

The Shape of Silicate Features in Semiregular and Mira Variables

FG Sge as a New–Born Carbon Star

Experimental Gas-Phase Spectroscopy of Carbon Molecular Structures and Diffuse Interstellar Bands

The Population of Red Giant Stars in Globular Clusters of the Fornax Dwarf Galaxy

Synthetic JHK Colors for M Dwarfs, M Giants, and Carbon Stars

Near-Infrared Spectroscopy of High Galactic Latitude Carbon Stars – They Might Be Giants?

A Simulation for a Carbon Star

On the Nature of Irregular Variables of Type Lb

Comparison of C-Rich Mira, Semiregular, and Irregular Variables

The Chemical Composition of the Halo Mira V CrB

Proceedings of the International Astronomical Union

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Symposium - International Astronomical Union, The Carbon Star Phenomenon

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