Coupling of thermal and nuclear modes at highly evolved stars
Abstract An analytical one-zone model (shell source) shows complex secular modes, if perturbations of chemical abundances are included. Very short periods (≲5a) can be calculated by choice of physically reasonable sets of parameters. Complex eigenvalues with unstable real parts may be regarded asthe...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Spindler, G. [verfasserIn] |
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| Format: |
Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
1979 |
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| Schlagwörter: |
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| Anmerkung: |
© D. Reidel Publishing Co 1979 |
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| Übergeordnetes Werk: |
Enthalten in: Astrophysics and space science - Kluwer Academic Publishers, 1968, 63(1979), 1 vom: Juni, Seite 237-245 |
|---|---|
| Übergeordnetes Werk: |
volume:63 ; year:1979 ; number:1 ; month:06 ; pages:237-245 |
| Links: |
|---|
| DOI / URN: |
10.1007/BF00647760 |
|---|
| Katalog-ID: |
OLC2066135828 |
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| 520 | |a Abstract An analytical one-zone model (shell source) shows complex secular modes, if perturbations of chemical abundances are included. Very short periods (≲5a) can be calculated by choice of physically reasonable sets of parameters. Complex eigenvalues with unstable real parts may be regarded asthermal instabilities with high frequency modulation of amplitude. | ||
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10.1007/BF00647760 doi (DE-627)OLC2066135828 (DE-He213)BF00647760-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Spindler, G. verfasserin aut Coupling of thermal and nuclear modes at highly evolved stars 1979 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Co 1979 Abstract An analytical one-zone model (shell source) shows complex secular modes, if perturbations of chemical abundances are included. Very short periods (≲5a) can be calculated by choice of physically reasonable sets of parameters. Complex eigenvalues with unstable real parts may be regarded asthermal instabilities with high frequency modulation of amplitude. Frequency Modulation Complex Eigenvalue High Frequency Modulation Nuclear Mode Chemical Abundance Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 63(1979), 1 vom: Juni, Seite 237-245 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:63 year:1979 number:1 month:06 pages:237-245 https://doi.org/10.1007/BF00647760 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OLC-DE-84 SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_24 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_4035 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4700 AR 63 1979 1 06 237-245 |
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10.1007/BF00647760 doi (DE-627)OLC2066135828 (DE-He213)BF00647760-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Spindler, G. verfasserin aut Coupling of thermal and nuclear modes at highly evolved stars 1979 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Co 1979 Abstract An analytical one-zone model (shell source) shows complex secular modes, if perturbations of chemical abundances are included. Very short periods (≲5a) can be calculated by choice of physically reasonable sets of parameters. Complex eigenvalues with unstable real parts may be regarded asthermal instabilities with high frequency modulation of amplitude. Frequency Modulation Complex Eigenvalue High Frequency Modulation Nuclear Mode Chemical Abundance Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 63(1979), 1 vom: Juni, Seite 237-245 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:63 year:1979 number:1 month:06 pages:237-245 https://doi.org/10.1007/BF00647760 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OLC-DE-84 SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_24 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_4035 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4700 AR 63 1979 1 06 237-245 |
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10.1007/BF00647760 doi (DE-627)OLC2066135828 (DE-He213)BF00647760-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Spindler, G. verfasserin aut Coupling of thermal and nuclear modes at highly evolved stars 1979 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Co 1979 Abstract An analytical one-zone model (shell source) shows complex secular modes, if perturbations of chemical abundances are included. Very short periods (≲5a) can be calculated by choice of physically reasonable sets of parameters. Complex eigenvalues with unstable real parts may be regarded asthermal instabilities with high frequency modulation of amplitude. Frequency Modulation Complex Eigenvalue High Frequency Modulation Nuclear Mode Chemical Abundance Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 63(1979), 1 vom: Juni, Seite 237-245 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:63 year:1979 number:1 month:06 pages:237-245 https://doi.org/10.1007/BF00647760 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OLC-DE-84 SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_24 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_4035 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4700 AR 63 1979 1 06 237-245 |
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10.1007/BF00647760 doi (DE-627)OLC2066135828 (DE-He213)BF00647760-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Spindler, G. verfasserin aut Coupling of thermal and nuclear modes at highly evolved stars 1979 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Co 1979 Abstract An analytical one-zone model (shell source) shows complex secular modes, if perturbations of chemical abundances are included. Very short periods (≲5a) can be calculated by choice of physically reasonable sets of parameters. Complex eigenvalues with unstable real parts may be regarded asthermal instabilities with high frequency modulation of amplitude. Frequency Modulation Complex Eigenvalue High Frequency Modulation Nuclear Mode Chemical Abundance Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 63(1979), 1 vom: Juni, Seite 237-245 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:63 year:1979 number:1 month:06 pages:237-245 https://doi.org/10.1007/BF00647760 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OLC-DE-84 SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_24 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_4035 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4700 AR 63 1979 1 06 237-245 |
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10.1007/BF00647760 doi (DE-627)OLC2066135828 (DE-He213)BF00647760-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Spindler, G. verfasserin aut Coupling of thermal and nuclear modes at highly evolved stars 1979 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Co 1979 Abstract An analytical one-zone model (shell source) shows complex secular modes, if perturbations of chemical abundances are included. Very short periods (≲5a) can be calculated by choice of physically reasonable sets of parameters. Complex eigenvalues with unstable real parts may be regarded asthermal instabilities with high frequency modulation of amplitude. Frequency Modulation Complex Eigenvalue High Frequency Modulation Nuclear Mode Chemical Abundance Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 63(1979), 1 vom: Juni, Seite 237-245 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:63 year:1979 number:1 month:06 pages:237-245 https://doi.org/10.1007/BF00647760 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OLC-DE-84 SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_24 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_4035 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4700 AR 63 1979 1 06 237-245 |
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coupling of thermal and nuclear modes at highly evolved stars |
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Coupling of thermal and nuclear modes at highly evolved stars |
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Abstract An analytical one-zone model (shell source) shows complex secular modes, if perturbations of chemical abundances are included. Very short periods (≲5a) can be calculated by choice of physically reasonable sets of parameters. Complex eigenvalues with unstable real parts may be regarded asthermal instabilities with high frequency modulation of amplitude. © D. Reidel Publishing Co 1979 |
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Abstract An analytical one-zone model (shell source) shows complex secular modes, if perturbations of chemical abundances are included. Very short periods (≲5a) can be calculated by choice of physically reasonable sets of parameters. Complex eigenvalues with unstable real parts may be regarded asthermal instabilities with high frequency modulation of amplitude. © D. Reidel Publishing Co 1979 |
| abstract_unstemmed |
Abstract An analytical one-zone model (shell source) shows complex secular modes, if perturbations of chemical abundances are included. Very short periods (≲5a) can be calculated by choice of physically reasonable sets of parameters. Complex eigenvalues with unstable real parts may be regarded asthermal instabilities with high frequency modulation of amplitude. © D. Reidel Publishing Co 1979 |
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Coupling of thermal and nuclear modes at highly evolved stars |
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