Gemini/GMOS spectra of globular clusters in the Virgo giant elliptical NGC 4649
- Autores
- Pierce, Michael; Bridges, Terry; Forbes, Duncan A.; Proctor, Robert; Beasley, Michael A.; Gebhardt, Karl; Faifer, Favio Raúl; Forte, Juan Carlos; Zepf, Stephen E.; Sharpies, Ray; Hanes, David A.
- Año de publicación
- 2006
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- NGC 4649 (M60) is one of a handful of giant Virgo ellipticals. We have obtained Gemini/GMOS (Gemini North Multi-Object Spectrograph) spectra for 38 globular clusters (GCs) associated with this galaxy. Applying the multi-index χ2 minimization technique of Proctor and Sansom with the single stellar population models of Thomas, Maraston and Korn, we derive ages, metallicities and α-element abundance ratios. We find several young (2-3 Gyr old) supersolar metallicity GCs, while the majority are old (>10 Gyr), spanning a range of metallicities from solar to [Z/H] = -2. At least two of these young GCs are at large projected radii of 17-20 kpc. The galaxy itself shows no obvious signs of a recent starburst, interaction or merger. A trend of decreasing α-element ratio with increasing metallicity is found.
Facultad de Ciencias Astronómicas y Geofísicas
Instituto de Astrofísica de La Plata - Materia
-
Ciencias Astronómicas
Galaxies: individual: NGC 4649
Galaxies: star clusters
Globular clusters: general - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by-nc-sa/4.0/
- Repositorio
.jpg)
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/84358
Ver los metadatos del registro completo
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Gemini/GMOS spectra of globular clusters in the Virgo giant elliptical NGC 4649Pierce, MichaelBridges, TerryForbes, Duncan A.Proctor, RobertBeasley, Michael A.Gebhardt, KarlFaifer, Favio RaúlForte, Juan CarlosZepf, Stephen E.Sharpies, RayHanes, David A.Ciencias AstronómicasGalaxies: individual: NGC 4649Galaxies: star clustersGlobular clusters: generalNGC 4649 (M60) is one of a handful of giant Virgo ellipticals. We have obtained Gemini/GMOS (Gemini North Multi-Object Spectrograph) spectra for 38 globular clusters (GCs) associated with this galaxy. Applying the multi-index χ<SUP>2</SUP> minimization technique of Proctor and Sansom with the single stellar population models of Thomas, Maraston and Korn, we derive ages, metallicities and α-element abundance ratios. We find several young (2-3 Gyr old) supersolar metallicity GCs, while the majority are old (>10 Gyr), spanning a range of metallicities from solar to [Z/H] = -2. At least two of these young GCs are at large projected radii of 17-20 kpc. The galaxy itself shows no obvious signs of a recent starburst, interaction or merger. A trend of decreasing α-element ratio with increasing metallicity is found.Facultad de Ciencias Astronómicas y GeofísicasInstituto de Astrofísica de La Plata2006info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf325-334http://sedici.unlp.edu.ar/handle/10915/84358enginfo:eu-repo/semantics/altIdentifier/issn/0035-8711info:eu-repo/semantics/altIdentifier/doi/10.1111/j.1365-2966.2006.10097.xinfo:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/4.0/Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-10-22T16:57:02Zoai:sedici.unlp.edu.ar:10915/84358Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-10-22 16:57:03.067SEDICI (UNLP) - Universidad Nacional de La Platafalse |
| dc.title.none.fl_str_mv |
Gemini/GMOS spectra of globular clusters in the Virgo giant elliptical NGC 4649 |
| title |
Gemini/GMOS spectra of globular clusters in the Virgo giant elliptical NGC 4649 |
| spellingShingle |
Gemini/GMOS spectra of globular clusters in the Virgo giant elliptical NGC 4649 Pierce, Michael Ciencias Astronómicas Galaxies: individual: NGC 4649 Galaxies: star clusters Globular clusters: general |
| title_short |
Gemini/GMOS spectra of globular clusters in the Virgo giant elliptical NGC 4649 |
| title_full |
Gemini/GMOS spectra of globular clusters in the Virgo giant elliptical NGC 4649 |
| title_fullStr |
Gemini/GMOS spectra of globular clusters in the Virgo giant elliptical NGC 4649 |
| title_full_unstemmed |
Gemini/GMOS spectra of globular clusters in the Virgo giant elliptical NGC 4649 |
| title_sort |
Gemini/GMOS spectra of globular clusters in the Virgo giant elliptical NGC 4649 |
| dc.creator.none.fl_str_mv |
Pierce, Michael Bridges, Terry Forbes, Duncan A. Proctor, Robert Beasley, Michael A. Gebhardt, Karl Faifer, Favio Raúl Forte, Juan Carlos Zepf, Stephen E. Sharpies, Ray Hanes, David A. |
| author |
Pierce, Michael |
| author_facet |
Pierce, Michael Bridges, Terry Forbes, Duncan A. Proctor, Robert Beasley, Michael A. Gebhardt, Karl Faifer, Favio Raúl Forte, Juan Carlos Zepf, Stephen E. Sharpies, Ray Hanes, David A. |
| author_role |
author |
| author2 |
Bridges, Terry Forbes, Duncan A. Proctor, Robert Beasley, Michael A. Gebhardt, Karl Faifer, Favio Raúl Forte, Juan Carlos Zepf, Stephen E. Sharpies, Ray Hanes, David A. |
| author2_role |
author author author author author author author author author author |
| dc.subject.none.fl_str_mv |
Ciencias Astronómicas Galaxies: individual: NGC 4649 Galaxies: star clusters Globular clusters: general |
| topic |
Ciencias Astronómicas Galaxies: individual: NGC 4649 Galaxies: star clusters Globular clusters: general |
| dc.description.none.fl_txt_mv |
NGC 4649 (M60) is one of a handful of giant Virgo ellipticals. We have obtained Gemini/GMOS (Gemini North Multi-Object Spectrograph) spectra for 38 globular clusters (GCs) associated with this galaxy. Applying the multi-index χ<SUP>2</SUP> minimization technique of Proctor and Sansom with the single stellar population models of Thomas, Maraston and Korn, we derive ages, metallicities and α-element abundance ratios. We find several young (2-3 Gyr old) supersolar metallicity GCs, while the majority are old (>10 Gyr), spanning a range of metallicities from solar to [Z/H] = -2. At least two of these young GCs are at large projected radii of 17-20 kpc. The galaxy itself shows no obvious signs of a recent starburst, interaction or merger. A trend of decreasing α-element ratio with increasing metallicity is found. Facultad de Ciencias Astronómicas y Geofísicas Instituto de Astrofísica de La Plata |
| description |
NGC 4649 (M60) is one of a handful of giant Virgo ellipticals. We have obtained Gemini/GMOS (Gemini North Multi-Object Spectrograph) spectra for 38 globular clusters (GCs) associated with this galaxy. Applying the multi-index χ<SUP>2</SUP> minimization technique of Proctor and Sansom with the single stellar population models of Thomas, Maraston and Korn, we derive ages, metallicities and α-element abundance ratios. We find several young (2-3 Gyr old) supersolar metallicity GCs, while the majority are old (>10 Gyr), spanning a range of metallicities from solar to [Z/H] = -2. At least two of these young GCs are at large projected radii of 17-20 kpc. The galaxy itself shows no obvious signs of a recent starburst, interaction or merger. A trend of decreasing α-element ratio with increasing metallicity is found. |
| publishDate |
2006 |
| dc.date.none.fl_str_mv |
2006 |
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info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion Articulo http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
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article |
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publishedVersion |
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http://sedici.unlp.edu.ar/handle/10915/84358 |
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http://sedici.unlp.edu.ar/handle/10915/84358 |
| dc.language.none.fl_str_mv |
eng |
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eng |
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info:eu-repo/semantics/altIdentifier/issn/0035-8711 info:eu-repo/semantics/altIdentifier/doi/10.1111/j.1365-2966.2006.10097.x |
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openAccess |
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http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
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