The possible protogalactic role of eddies in a turbulent early universe
Abstract It is shown that eddies, present in a turbulent early universe, can form excellent galaxies upon collapse of the eddies and a small amount of viscous evolution. The resulting model galaxies display realistically flat rotation curves as well as exponential-like luminosity profiles. The dark...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Brown, Wilbur K. [verfasserIn] |
|---|
| Format: |
Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
1985 |
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| Schlagwörter: |
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| Anmerkung: |
© D. Reidel Publishing Company 1985 |
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| Übergeordnetes Werk: |
Enthalten in: Astrophysics and space science - Kluwer Academic Publishers, 1968, 115(1985), 2 vom: Okt., Seite 257-265 |
|---|---|
| Übergeordnetes Werk: |
volume:115 ; year:1985 ; number:2 ; month:10 ; pages:257-265 |
| Links: |
|---|
| DOI / URN: |
10.1007/BF00653804 |
|---|
| Katalog-ID: |
OLC206615797X |
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| 520 | |a Abstract It is shown that eddies, present in a turbulent early universe, can form excellent galaxies upon collapse of the eddies and a small amount of viscous evolution. The resulting model galaxies display realistically flat rotation curves as well as exponential-like luminosity profiles. The dark mass is allowed to be non-baryonic in this model. | ||
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10.1007/BF00653804 doi (DE-627)OLC206615797X (DE-He213)BF00653804-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Brown, Wilbur K. verfasserin aut The possible protogalactic role of eddies in a turbulent early universe 1985 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1985 Abstract It is shown that eddies, present in a turbulent early universe, can form excellent galaxies upon collapse of the eddies and a small amount of viscous evolution. The resulting model galaxies display realistically flat rotation curves as well as exponential-like luminosity profiles. The dark mass is allowed to be non-baryonic in this model. Early Universe Rotation Curve Model Galaxy Dark Mass Flat Rotation Curve Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 115(1985), 2 vom: Okt., Seite 257-265 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:115 year:1985 number:2 month:10 pages:257-265 https://doi.org/10.1007/BF00653804 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_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_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4700 AR 115 1985 2 10 257-265 |
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10.1007/BF00653804 doi (DE-627)OLC206615797X (DE-He213)BF00653804-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Brown, Wilbur K. verfasserin aut The possible protogalactic role of eddies in a turbulent early universe 1985 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1985 Abstract It is shown that eddies, present in a turbulent early universe, can form excellent galaxies upon collapse of the eddies and a small amount of viscous evolution. The resulting model galaxies display realistically flat rotation curves as well as exponential-like luminosity profiles. The dark mass is allowed to be non-baryonic in this model. Early Universe Rotation Curve Model Galaxy Dark Mass Flat Rotation Curve Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 115(1985), 2 vom: Okt., Seite 257-265 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:115 year:1985 number:2 month:10 pages:257-265 https://doi.org/10.1007/BF00653804 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_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_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4700 AR 115 1985 2 10 257-265 |
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The possible protogalactic role of eddies in a turbulent early universe |
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Abstract It is shown that eddies, present in a turbulent early universe, can form excellent galaxies upon collapse of the eddies and a small amount of viscous evolution. The resulting model galaxies display realistically flat rotation curves as well as exponential-like luminosity profiles. The dark mass is allowed to be non-baryonic in this model. © D. Reidel Publishing Company 1985 |
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Abstract It is shown that eddies, present in a turbulent early universe, can form excellent galaxies upon collapse of the eddies and a small amount of viscous evolution. The resulting model galaxies display realistically flat rotation curves as well as exponential-like luminosity profiles. The dark mass is allowed to be non-baryonic in this model. © D. Reidel Publishing Company 1985 |
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Abstract It is shown that eddies, present in a turbulent early universe, can form excellent galaxies upon collapse of the eddies and a small amount of viscous evolution. The resulting model galaxies display realistically flat rotation curves as well as exponential-like luminosity profiles. The dark mass is allowed to be non-baryonic in this model. © D. Reidel Publishing Company 1985 |
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The possible protogalactic role of eddies in a turbulent early universe |
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https://doi.org/10.1007/BF00653804 |
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2024-07-04T03:53:15.452Z |
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