Tentative Detection of Circumstellar CO2 from the AGB Star R Crateris
Abstract We report on and discuss the detection of an emission feature at 14.98 µm from the oxygen-rich, semi-regularly pulsating Asymptotic Giant Branch star R Crateris, a feature which we suggest to be due to the 01 Q-branch of circumstellar CO2. We also suggest a reasonable excitation mechanism,...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Ryde, N. [verfasserIn] |
|---|
| Format: |
Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
1997 |
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| Schlagwörter: |
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| Anmerkung: |
© Kluwer Academic Publishers 1997 |
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| Übergeordnetes Werk: |
Enthalten in: Astrophysics and space science - Kluwer Academic Publishers, 1968, 255(1997), 1-2 vom: Jan., Seite 301-302 |
|---|---|
| Übergeordnetes Werk: |
volume:255 ; year:1997 ; number:1-2 ; month:01 ; pages:301-302 |
| Links: |
|---|
| DOI / URN: |
10.1023/A:1001583606843 |
|---|
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OLC2066213187 |
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| 520 | |a Abstract We report on and discuss the detection of an emission feature at 14.98 µm from the oxygen-rich, semi-regularly pulsating Asymptotic Giant Branch star R Crateris, a feature which we suggest to be due to the 01 Q-branch of circumstellar CO2. We also suggest a reasonable excitation mechanism, which could explain the height, the width and the asymmetry of the feature. | ||
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| 700 | 1 | |a Olofsson, H. |4 aut | |
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10.1023/A:1001583606843 doi (DE-627)OLC2066213187 (DE-He213)A:1001583606843-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Ryde, N. verfasserin aut Tentative Detection of Circumstellar CO2 from the AGB Star R Crateris 1997 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1997 Abstract We report on and discuss the detection of an emission feature at 14.98 µm from the oxygen-rich, semi-regularly pulsating Asymptotic Giant Branch star R Crateris, a feature which we suggest to be due to the 01 Q-branch of circumstellar CO2. We also suggest a reasonable excitation mechanism, which could explain the height, the width and the asymmetry of the feature. Emission Feature Excitation Mechanism Asymptotic Giant Branch Star Branch Star Asymptotic Giant Eriksson, K. aut Gustafsson, B. aut Lindqvist, M. aut Olofsson, H. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 255(1997), 1-2 vom: Jan., Seite 301-302 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:255 year:1997 number:1-2 month:01 pages:301-302 https://doi.org/10.1023/A:1001583606843 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4027 GBV_ILN_4046 AR 255 1997 1-2 01 301-302 |
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10.1023/A:1001583606843 doi (DE-627)OLC2066213187 (DE-He213)A:1001583606843-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Ryde, N. verfasserin aut Tentative Detection of Circumstellar CO2 from the AGB Star R Crateris 1997 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1997 Abstract We report on and discuss the detection of an emission feature at 14.98 µm from the oxygen-rich, semi-regularly pulsating Asymptotic Giant Branch star R Crateris, a feature which we suggest to be due to the 01 Q-branch of circumstellar CO2. We also suggest a reasonable excitation mechanism, which could explain the height, the width and the asymmetry of the feature. Emission Feature Excitation Mechanism Asymptotic Giant Branch Star Branch Star Asymptotic Giant Eriksson, K. aut Gustafsson, B. aut Lindqvist, M. aut Olofsson, H. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 255(1997), 1-2 vom: Jan., Seite 301-302 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:255 year:1997 number:1-2 month:01 pages:301-302 https://doi.org/10.1023/A:1001583606843 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4027 GBV_ILN_4046 AR 255 1997 1-2 01 301-302 |
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tentative detection of circumstellar co2 from the agb star r crateris |
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Tentative Detection of Circumstellar CO2 from the AGB Star R Crateris |
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Abstract We report on and discuss the detection of an emission feature at 14.98 µm from the oxygen-rich, semi-regularly pulsating Asymptotic Giant Branch star R Crateris, a feature which we suggest to be due to the 01 Q-branch of circumstellar CO2. We also suggest a reasonable excitation mechanism, which could explain the height, the width and the asymmetry of the feature. © Kluwer Academic Publishers 1997 |
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Abstract We report on and discuss the detection of an emission feature at 14.98 µm from the oxygen-rich, semi-regularly pulsating Asymptotic Giant Branch star R Crateris, a feature which we suggest to be due to the 01 Q-branch of circumstellar CO2. We also suggest a reasonable excitation mechanism, which could explain the height, the width and the asymmetry of the feature. © Kluwer Academic Publishers 1997 |
| abstract_unstemmed |
Abstract We report on and discuss the detection of an emission feature at 14.98 µm from the oxygen-rich, semi-regularly pulsating Asymptotic Giant Branch star R Crateris, a feature which we suggest to be due to the 01 Q-branch of circumstellar CO2. We also suggest a reasonable excitation mechanism, which could explain the height, the width and the asymmetry of the feature. © Kluwer Academic Publishers 1997 |
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Tentative Detection of Circumstellar CO2 from the AGB Star R Crateris |
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Eriksson, K. Gustafsson, B. Lindqvist, M. Olofsson, H. |
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