Kinematics and Dynamics of the Galactic Stellar Halo
Abstract The structure, kinematics and dynamics of the Galactic stellar halo are reviewed including evidence of substructure in the spatial distribution and kinematics of halo stars. Implications for galaxy formation theory are subsequently discussed; in particular it is argued that the observed kin...
Ausführliche Beschreibung
Autor*in: |
Sommer-Larsen, Jesper [verfasserIn] |
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Format: |
Artikel |
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Sprache: |
Englisch |
Erschienen: |
1999 |
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Schlagwörter: |
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Anmerkung: |
© Kluwer Academic Publishers 1999 |
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Übergeordnetes Werk: |
Enthalten in: Astrophysics and space science - Kluwer Academic Publishers, 1968, 265(1999), 1-4 vom: Juli, Seite 123-131 |
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Übergeordnetes Werk: |
volume:265 ; year:1999 ; number:1-4 ; month:07 ; pages:123-131 |
Links: |
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DOI / URN: |
10.1023/A:1002114216496 |
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Katalog-ID: |
OLC2066219711 |
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10.1023/A:1002114216496 doi (DE-627)OLC2066219711 (DE-He213)A:1002114216496-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Sommer-Larsen, Jesper verfasserin aut Kinematics and Dynamics of the Galactic Stellar Halo 1999 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1999 Abstract The structure, kinematics and dynamics of the Galactic stellar halo are reviewed including evidence of substructure in the spatial distribution and kinematics of halo stars. Implications for galaxy formation theory are subsequently discussed; in particular it is argued that the observed kinematics of stars in the outer Galactic halo can be used as an important constraint on viable galaxy formation scenarios. Dark Matter Disk Galaxy Galactic Halo Dark Matter Halo Galactocentric Distance Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 265(1999), 1-4 vom: Juli, Seite 123-131 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:265 year:1999 number:1-4 month:07 pages:123-131 https://doi.org/10.1023/A:1002114216496 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 GBV_ILN_4046 AR 265 1999 1-4 07 123-131 |
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10.1023/A:1002114216496 doi (DE-627)OLC2066219711 (DE-He213)A:1002114216496-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Sommer-Larsen, Jesper verfasserin aut Kinematics and Dynamics of the Galactic Stellar Halo 1999 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1999 Abstract The structure, kinematics and dynamics of the Galactic stellar halo are reviewed including evidence of substructure in the spatial distribution and kinematics of halo stars. Implications for galaxy formation theory are subsequently discussed; in particular it is argued that the observed kinematics of stars in the outer Galactic halo can be used as an important constraint on viable galaxy formation scenarios. Dark Matter Disk Galaxy Galactic Halo Dark Matter Halo Galactocentric Distance Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 265(1999), 1-4 vom: Juli, Seite 123-131 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:265 year:1999 number:1-4 month:07 pages:123-131 https://doi.org/10.1023/A:1002114216496 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 GBV_ILN_4046 AR 265 1999 1-4 07 123-131 |
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10.1023/A:1002114216496 doi (DE-627)OLC2066219711 (DE-He213)A:1002114216496-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Sommer-Larsen, Jesper verfasserin aut Kinematics and Dynamics of the Galactic Stellar Halo 1999 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1999 Abstract The structure, kinematics and dynamics of the Galactic stellar halo are reviewed including evidence of substructure in the spatial distribution and kinematics of halo stars. Implications for galaxy formation theory are subsequently discussed; in particular it is argued that the observed kinematics of stars in the outer Galactic halo can be used as an important constraint on viable galaxy formation scenarios. Dark Matter Disk Galaxy Galactic Halo Dark Matter Halo Galactocentric Distance Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 265(1999), 1-4 vom: Juli, Seite 123-131 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:265 year:1999 number:1-4 month:07 pages:123-131 https://doi.org/10.1023/A:1002114216496 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 GBV_ILN_4046 AR 265 1999 1-4 07 123-131 |
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Abstract The structure, kinematics and dynamics of the Galactic stellar halo are reviewed including evidence of substructure in the spatial distribution and kinematics of halo stars. Implications for galaxy formation theory are subsequently discussed; in particular it is argued that the observed kinematics of stars in the outer Galactic halo can be used as an important constraint on viable galaxy formation scenarios. © Kluwer Academic Publishers 1999 |
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Abstract The structure, kinematics and dynamics of the Galactic stellar halo are reviewed including evidence of substructure in the spatial distribution and kinematics of halo stars. Implications for galaxy formation theory are subsequently discussed; in particular it is argued that the observed kinematics of stars in the outer Galactic halo can be used as an important constraint on viable galaxy formation scenarios. © Kluwer Academic Publishers 1999 |
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Abstract The structure, kinematics and dynamics of the Galactic stellar halo are reviewed including evidence of substructure in the spatial distribution and kinematics of halo stars. Implications for galaxy formation theory are subsequently discussed; in particular it is argued that the observed kinematics of stars in the outer Galactic halo can be used as an important constraint on viable galaxy formation scenarios. © Kluwer Academic Publishers 1999 |
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