Old stellar systems in UV: resolved and integrated properties
Abstract The UV properties of old stellar populations have been subject of intense scrutiny from the late sixties, when the UV-upturn in early type galaxies was first discovered. Because of their proximity and relative simplicity, Galactic globular clusters (GGCs) are ideal local templates to unders...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Dalessandro, E. [verfasserIn] |
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| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2014 |
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| Schlagwörter: |
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| Anmerkung: |
© Springer Science+Business Media Dordrecht 2014 |
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| Übergeordnetes Werk: |
Enthalten in: Astrophysics and space science - Springer Netherlands, 1968, 354(2014), 1 vom: 28. Mai, Seite 47-54 |
|---|---|
| Übergeordnetes Werk: |
volume:354 ; year:2014 ; number:1 ; day:28 ; month:05 ; pages:47-54 |
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| DOI / URN: |
10.1007/s10509-014-1974-z |
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| 520 | |a Abstract The UV properties of old stellar populations have been subject of intense scrutiny from the late sixties, when the UV-upturn in early type galaxies was first discovered. Because of their proximity and relative simplicity, Galactic globular clusters (GGCs) are ideal local templates to understand how the integrated UV light is driven by hot stellar populations, primarily horizontal branch stars and their progeny. Our understanding of such stars is still plagued by theoretical uncertainties, which are partly due to the absence of an accurate, comprehensive, statistically representative homogeneous data-set. To move a step forward on this subject, we have combined the HST and GALEX capabilities and collected the largest data-base ever obtained for GGCs in UV. This data-base is best suited to provide insights on the HB second parameter problem and on the first stages of GCs formation and chemical evolution and to understand how they are linked to the observed properties of extragalactic systems. | ||
| 650 | 4 | |a Globular clusters: UV properties | |
| 650 | 4 | |a Horizontal Branch | |
| 650 | 4 | |a Integrated colours | |
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10.1007/s10509-014-1974-z doi (DE-627)OLC2066276200 (DE-He213)s10509-014-1974-z-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Dalessandro, E. verfasserin aut Old stellar systems in UV: resolved and integrated properties 2014 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media Dordrecht 2014 Abstract The UV properties of old stellar populations have been subject of intense scrutiny from the late sixties, when the UV-upturn in early type galaxies was first discovered. Because of their proximity and relative simplicity, Galactic globular clusters (GGCs) are ideal local templates to understand how the integrated UV light is driven by hot stellar populations, primarily horizontal branch stars and their progeny. Our understanding of such stars is still plagued by theoretical uncertainties, which are partly due to the absence of an accurate, comprehensive, statistically representative homogeneous data-set. To move a step forward on this subject, we have combined the HST and GALEX capabilities and collected the largest data-base ever obtained for GGCs in UV. This data-base is best suited to provide insights on the HB second parameter problem and on the first stages of GCs formation and chemical evolution and to understand how they are linked to the observed properties of extragalactic systems. Globular clusters: UV properties Horizontal Branch Integrated colours Enthalten in Astrophysics and space science Springer Netherlands, 1968 354(2014), 1 vom: 28. Mai, Seite 47-54 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:354 year:2014 number:1 day:28 month:05 pages:47-54 https://doi.org/10.1007/s10509-014-1974-z lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_4012 AR 354 2014 1 28 05 47-54 |
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10.1007/s10509-014-1974-z doi (DE-627)OLC2066276200 (DE-He213)s10509-014-1974-z-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Dalessandro, E. verfasserin aut Old stellar systems in UV: resolved and integrated properties 2014 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media Dordrecht 2014 Abstract The UV properties of old stellar populations have been subject of intense scrutiny from the late sixties, when the UV-upturn in early type galaxies was first discovered. Because of their proximity and relative simplicity, Galactic globular clusters (GGCs) are ideal local templates to understand how the integrated UV light is driven by hot stellar populations, primarily horizontal branch stars and their progeny. Our understanding of such stars is still plagued by theoretical uncertainties, which are partly due to the absence of an accurate, comprehensive, statistically representative homogeneous data-set. To move a step forward on this subject, we have combined the HST and GALEX capabilities and collected the largest data-base ever obtained for GGCs in UV. This data-base is best suited to provide insights on the HB second parameter problem and on the first stages of GCs formation and chemical evolution and to understand how they are linked to the observed properties of extragalactic systems. Globular clusters: UV properties Horizontal Branch Integrated colours Enthalten in Astrophysics and space science Springer Netherlands, 1968 354(2014), 1 vom: 28. Mai, Seite 47-54 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:354 year:2014 number:1 day:28 month:05 pages:47-54 https://doi.org/10.1007/s10509-014-1974-z lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_4012 AR 354 2014 1 28 05 47-54 |
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10.1007/s10509-014-1974-z doi (DE-627)OLC2066276200 (DE-He213)s10509-014-1974-z-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Dalessandro, E. verfasserin aut Old stellar systems in UV: resolved and integrated properties 2014 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media Dordrecht 2014 Abstract The UV properties of old stellar populations have been subject of intense scrutiny from the late sixties, when the UV-upturn in early type galaxies was first discovered. Because of their proximity and relative simplicity, Galactic globular clusters (GGCs) are ideal local templates to understand how the integrated UV light is driven by hot stellar populations, primarily horizontal branch stars and their progeny. Our understanding of such stars is still plagued by theoretical uncertainties, which are partly due to the absence of an accurate, comprehensive, statistically representative homogeneous data-set. To move a step forward on this subject, we have combined the HST and GALEX capabilities and collected the largest data-base ever obtained for GGCs in UV. This data-base is best suited to provide insights on the HB second parameter problem and on the first stages of GCs formation and chemical evolution and to understand how they are linked to the observed properties of extragalactic systems. Globular clusters: UV properties Horizontal Branch Integrated colours Enthalten in Astrophysics and space science Springer Netherlands, 1968 354(2014), 1 vom: 28. Mai, Seite 47-54 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:354 year:2014 number:1 day:28 month:05 pages:47-54 https://doi.org/10.1007/s10509-014-1974-z lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_4012 AR 354 2014 1 28 05 47-54 |
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10.1007/s10509-014-1974-z doi (DE-627)OLC2066276200 (DE-He213)s10509-014-1974-z-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Dalessandro, E. verfasserin aut Old stellar systems in UV: resolved and integrated properties 2014 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media Dordrecht 2014 Abstract The UV properties of old stellar populations have been subject of intense scrutiny from the late sixties, when the UV-upturn in early type galaxies was first discovered. Because of their proximity and relative simplicity, Galactic globular clusters (GGCs) are ideal local templates to understand how the integrated UV light is driven by hot stellar populations, primarily horizontal branch stars and their progeny. Our understanding of such stars is still plagued by theoretical uncertainties, which are partly due to the absence of an accurate, comprehensive, statistically representative homogeneous data-set. To move a step forward on this subject, we have combined the HST and GALEX capabilities and collected the largest data-base ever obtained for GGCs in UV. This data-base is best suited to provide insights on the HB second parameter problem and on the first stages of GCs formation and chemical evolution and to understand how they are linked to the observed properties of extragalactic systems. Globular clusters: UV properties Horizontal Branch Integrated colours Enthalten in Astrophysics and space science Springer Netherlands, 1968 354(2014), 1 vom: 28. Mai, Seite 47-54 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:354 year:2014 number:1 day:28 month:05 pages:47-54 https://doi.org/10.1007/s10509-014-1974-z lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_4012 AR 354 2014 1 28 05 47-54 |
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10.1007/s10509-014-1974-z doi (DE-627)OLC2066276200 (DE-He213)s10509-014-1974-z-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Dalessandro, E. verfasserin aut Old stellar systems in UV: resolved and integrated properties 2014 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media Dordrecht 2014 Abstract The UV properties of old stellar populations have been subject of intense scrutiny from the late sixties, when the UV-upturn in early type galaxies was first discovered. Because of their proximity and relative simplicity, Galactic globular clusters (GGCs) are ideal local templates to understand how the integrated UV light is driven by hot stellar populations, primarily horizontal branch stars and their progeny. Our understanding of such stars is still plagued by theoretical uncertainties, which are partly due to the absence of an accurate, comprehensive, statistically representative homogeneous data-set. To move a step forward on this subject, we have combined the HST and GALEX capabilities and collected the largest data-base ever obtained for GGCs in UV. This data-base is best suited to provide insights on the HB second parameter problem and on the first stages of GCs formation and chemical evolution and to understand how they are linked to the observed properties of extragalactic systems. Globular clusters: UV properties Horizontal Branch Integrated colours Enthalten in Astrophysics and space science Springer Netherlands, 1968 354(2014), 1 vom: 28. Mai, Seite 47-54 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:354 year:2014 number:1 day:28 month:05 pages:47-54 https://doi.org/10.1007/s10509-014-1974-z lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_4012 AR 354 2014 1 28 05 47-54 |
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Abstract The UV properties of old stellar populations have been subject of intense scrutiny from the late sixties, when the UV-upturn in early type galaxies was first discovered. Because of their proximity and relative simplicity, Galactic globular clusters (GGCs) are ideal local templates to understand how the integrated UV light is driven by hot stellar populations, primarily horizontal branch stars and their progeny. Our understanding of such stars is still plagued by theoretical uncertainties, which are partly due to the absence of an accurate, comprehensive, statistically representative homogeneous data-set. To move a step forward on this subject, we have combined the HST and GALEX capabilities and collected the largest data-base ever obtained for GGCs in UV. This data-base is best suited to provide insights on the HB second parameter problem and on the first stages of GCs formation and chemical evolution and to understand how they are linked to the observed properties of extragalactic systems. © Springer Science+Business Media Dordrecht 2014 |
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Abstract The UV properties of old stellar populations have been subject of intense scrutiny from the late sixties, when the UV-upturn in early type galaxies was first discovered. Because of their proximity and relative simplicity, Galactic globular clusters (GGCs) are ideal local templates to understand how the integrated UV light is driven by hot stellar populations, primarily horizontal branch stars and their progeny. Our understanding of such stars is still plagued by theoretical uncertainties, which are partly due to the absence of an accurate, comprehensive, statistically representative homogeneous data-set. To move a step forward on this subject, we have combined the HST and GALEX capabilities and collected the largest data-base ever obtained for GGCs in UV. This data-base is best suited to provide insights on the HB second parameter problem and on the first stages of GCs formation and chemical evolution and to understand how they are linked to the observed properties of extragalactic systems. © Springer Science+Business Media Dordrecht 2014 |
| abstract_unstemmed |
Abstract The UV properties of old stellar populations have been subject of intense scrutiny from the late sixties, when the UV-upturn in early type galaxies was first discovered. Because of their proximity and relative simplicity, Galactic globular clusters (GGCs) are ideal local templates to understand how the integrated UV light is driven by hot stellar populations, primarily horizontal branch stars and their progeny. Our understanding of such stars is still plagued by theoretical uncertainties, which are partly due to the absence of an accurate, comprehensive, statistically representative homogeneous data-set. To move a step forward on this subject, we have combined the HST and GALEX capabilities and collected the largest data-base ever obtained for GGCs in UV. This data-base is best suited to provide insights on the HB second parameter problem and on the first stages of GCs formation and chemical evolution and to understand how they are linked to the observed properties of extragalactic systems. © Springer Science+Business Media Dordrecht 2014 |
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| title_short |
Old stellar systems in UV: resolved and integrated properties |
| url |
https://doi.org/10.1007/s10509-014-1974-z |
| remote_bool |
false |
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129062723 |
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n |
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| doi_str |
10.1007/s10509-014-1974-z |
| up_date |
2024-07-04T04:08:01.541Z |
| _version_ |
1803620011529469952 |
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Because of their proximity and relative simplicity, Galactic globular clusters (GGCs) are ideal local templates to understand how the integrated UV light is driven by hot stellar populations, primarily horizontal branch stars and their progeny. Our understanding of such stars is still plagued by theoretical uncertainties, which are partly due to the absence of an accurate, comprehensive, statistically representative homogeneous data-set. To move a step forward on this subject, we have combined the HST and GALEX capabilities and collected the largest data-base ever obtained for GGCs in UV. 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