Modeling the Star Formation in Galaxies Using the Chemo-DynamicalSPH Code
Abstract A new Chemo-Dynamical Smoothed Particle Hydrodynamic (CD-SPH) code is presented. The disk galaxy is described as a multi-fragmented gas and star system, embedded in a cold dark matter halo. The star formation (SF) process, SNII, SNIa and PN events as well as chemical enrichment of gas have...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Berczik, Peter [verfasserIn] |
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| Format: |
Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
2000 |
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| Schlagwörter: |
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| Anmerkung: |
© Kluwer Academic Publishers 2000 |
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| Übergeordnetes Werk: |
Enthalten in: Astrophysics and space science - Kluwer Academic Publishers, 1968, 271(2000), 2 vom: März, Seite 103-126 |
|---|---|
| Übergeordnetes Werk: |
volume:271 ; year:2000 ; number:2 ; month:03 ; pages:103-126 |
| Links: |
|---|
| DOI / URN: |
10.1023/A:1002485702347 |
|---|
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OLC206622300X |
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| 520 | |a Abstract A new Chemo-Dynamical Smoothed Particle Hydrodynamic (CD-SPH) code is presented. The disk galaxy is described as a multi-fragmented gas and star system, embedded in a cold dark matter halo. The star formation (SF) process, SNII, SNIa and PN events as well as chemical enrichment of gas have been considered within the framework of the standard SPH model. Using this model we describe the dynamical and chemical evolution of triaxial disk-like galaxies. It is found that such approach provides a realistic description of the process of formation, chemical and dynamical evolution of disk galaxies over a cosmological timescale. | ||
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| 650 | 4 | |a Smooth Particle Hydrodynamic | |
| 650 | 4 | |a Disk Galaxy | |
| 650 | 4 | |a Smooth Particle Hydrodynamic Method | |
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10.1023/A:1002485702347 doi (DE-627)OLC206622300X (DE-He213)A:1002485702347-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Berczik, Peter verfasserin aut Modeling the Star Formation in Galaxies Using the Chemo-DynamicalSPH Code 2000 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 2000 Abstract A new Chemo-Dynamical Smoothed Particle Hydrodynamic (CD-SPH) code is presented. The disk galaxy is described as a multi-fragmented gas and star system, embedded in a cold dark matter halo. The star formation (SF) process, SNII, SNIa and PN events as well as chemical enrichment of gas have been considered within the framework of the standard SPH model. Using this model we describe the dynamical and chemical evolution of triaxial disk-like galaxies. It is found that such approach provides a realistic description of the process of formation, chemical and dynamical evolution of disk galaxies over a cosmological timescale. Smooth Particle Hydrodynamic Chaotic Motion Smooth Particle Hydrodynamic Disk Galaxy Smooth Particle Hydrodynamic Method Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 271(2000), 2 vom: März, Seite 103-126 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:271 year:2000 number:2 month:03 pages:103-126 https://doi.org/10.1023/A:1002485702347 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_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 AR 271 2000 2 03 103-126 |
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10.1023/A:1002485702347 doi (DE-627)OLC206622300X (DE-He213)A:1002485702347-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Berczik, Peter verfasserin aut Modeling the Star Formation in Galaxies Using the Chemo-DynamicalSPH Code 2000 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 2000 Abstract A new Chemo-Dynamical Smoothed Particle Hydrodynamic (CD-SPH) code is presented. The disk galaxy is described as a multi-fragmented gas and star system, embedded in a cold dark matter halo. The star formation (SF) process, SNII, SNIa and PN events as well as chemical enrichment of gas have been considered within the framework of the standard SPH model. Using this model we describe the dynamical and chemical evolution of triaxial disk-like galaxies. It is found that such approach provides a realistic description of the process of formation, chemical and dynamical evolution of disk galaxies over a cosmological timescale. Smooth Particle Hydrodynamic Chaotic Motion Smooth Particle Hydrodynamic Disk Galaxy Smooth Particle Hydrodynamic Method Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 271(2000), 2 vom: März, Seite 103-126 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:271 year:2000 number:2 month:03 pages:103-126 https://doi.org/10.1023/A:1002485702347 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_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 AR 271 2000 2 03 103-126 |
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10.1023/A:1002485702347 doi (DE-627)OLC206622300X (DE-He213)A:1002485702347-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Berczik, Peter verfasserin aut Modeling the Star Formation in Galaxies Using the Chemo-DynamicalSPH Code 2000 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 2000 Abstract A new Chemo-Dynamical Smoothed Particle Hydrodynamic (CD-SPH) code is presented. The disk galaxy is described as a multi-fragmented gas and star system, embedded in a cold dark matter halo. The star formation (SF) process, SNII, SNIa and PN events as well as chemical enrichment of gas have been considered within the framework of the standard SPH model. Using this model we describe the dynamical and chemical evolution of triaxial disk-like galaxies. It is found that such approach provides a realistic description of the process of formation, chemical and dynamical evolution of disk galaxies over a cosmological timescale. Smooth Particle Hydrodynamic Chaotic Motion Smooth Particle Hydrodynamic Disk Galaxy Smooth Particle Hydrodynamic Method Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 271(2000), 2 vom: März, Seite 103-126 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:271 year:2000 number:2 month:03 pages:103-126 https://doi.org/10.1023/A:1002485702347 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_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 AR 271 2000 2 03 103-126 |
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10.1023/A:1002485702347 doi (DE-627)OLC206622300X (DE-He213)A:1002485702347-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Berczik, Peter verfasserin aut Modeling the Star Formation in Galaxies Using the Chemo-DynamicalSPH Code 2000 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 2000 Abstract A new Chemo-Dynamical Smoothed Particle Hydrodynamic (CD-SPH) code is presented. The disk galaxy is described as a multi-fragmented gas and star system, embedded in a cold dark matter halo. The star formation (SF) process, SNII, SNIa and PN events as well as chemical enrichment of gas have been considered within the framework of the standard SPH model. Using this model we describe the dynamical and chemical evolution of triaxial disk-like galaxies. It is found that such approach provides a realistic description of the process of formation, chemical and dynamical evolution of disk galaxies over a cosmological timescale. Smooth Particle Hydrodynamic Chaotic Motion Smooth Particle Hydrodynamic Disk Galaxy Smooth Particle Hydrodynamic Method Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 271(2000), 2 vom: März, Seite 103-126 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:271 year:2000 number:2 month:03 pages:103-126 https://doi.org/10.1023/A:1002485702347 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_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 AR 271 2000 2 03 103-126 |
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10.1023/A:1002485702347 doi (DE-627)OLC206622300X (DE-He213)A:1002485702347-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Berczik, Peter verfasserin aut Modeling the Star Formation in Galaxies Using the Chemo-DynamicalSPH Code 2000 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 2000 Abstract A new Chemo-Dynamical Smoothed Particle Hydrodynamic (CD-SPH) code is presented. The disk galaxy is described as a multi-fragmented gas and star system, embedded in a cold dark matter halo. The star formation (SF) process, SNII, SNIa and PN events as well as chemical enrichment of gas have been considered within the framework of the standard SPH model. Using this model we describe the dynamical and chemical evolution of triaxial disk-like galaxies. It is found that such approach provides a realistic description of the process of formation, chemical and dynamical evolution of disk galaxies over a cosmological timescale. Smooth Particle Hydrodynamic Chaotic Motion Smooth Particle Hydrodynamic Disk Galaxy Smooth Particle Hydrodynamic Method Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 271(2000), 2 vom: März, Seite 103-126 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:271 year:2000 number:2 month:03 pages:103-126 https://doi.org/10.1023/A:1002485702347 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_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 AR 271 2000 2 03 103-126 |
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Modeling the Star Formation in Galaxies Using the Chemo-DynamicalSPH Code |
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Abstract A new Chemo-Dynamical Smoothed Particle Hydrodynamic (CD-SPH) code is presented. The disk galaxy is described as a multi-fragmented gas and star system, embedded in a cold dark matter halo. The star formation (SF) process, SNII, SNIa and PN events as well as chemical enrichment of gas have been considered within the framework of the standard SPH model. Using this model we describe the dynamical and chemical evolution of triaxial disk-like galaxies. It is found that such approach provides a realistic description of the process of formation, chemical and dynamical evolution of disk galaxies over a cosmological timescale. © Kluwer Academic Publishers 2000 |
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Abstract A new Chemo-Dynamical Smoothed Particle Hydrodynamic (CD-SPH) code is presented. The disk galaxy is described as a multi-fragmented gas and star system, embedded in a cold dark matter halo. The star formation (SF) process, SNII, SNIa and PN events as well as chemical enrichment of gas have been considered within the framework of the standard SPH model. Using this model we describe the dynamical and chemical evolution of triaxial disk-like galaxies. It is found that such approach provides a realistic description of the process of formation, chemical and dynamical evolution of disk galaxies over a cosmological timescale. © Kluwer Academic Publishers 2000 |
| abstract_unstemmed |
Abstract A new Chemo-Dynamical Smoothed Particle Hydrodynamic (CD-SPH) code is presented. The disk galaxy is described as a multi-fragmented gas and star system, embedded in a cold dark matter halo. The star formation (SF) process, SNII, SNIa and PN events as well as chemical enrichment of gas have been considered within the framework of the standard SPH model. Using this model we describe the dynamical and chemical evolution of triaxial disk-like galaxies. It is found that such approach provides a realistic description of the process of formation, chemical and dynamical evolution of disk galaxies over a cosmological timescale. © Kluwer Academic Publishers 2000 |
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Modeling the Star Formation in Galaxies Using the Chemo-DynamicalSPH Code |
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