Using the Age and Metallicity of 8 Star Clusters to confirm the Chemical Enrichment History of the LMC
In this paper, we find the ages and metallicities of 8 Large Magellanic Cloud (LMC) star clusters obtained from integrated light spectra and use them to obtain the Chemical Enrichment History of the host galaxy. Our results are in good agreement with those obtained from resolved studies. This confir...
محفوظ في:
| المؤلف الرئيسي: | |
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| مؤلفون آخرون: | , , |
| التنسيق: | article |
| منشور في: |
2019
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| الوصول للمادة أونلاين: | http://hdl.handle.net/11073/16614 |
| الوسوم: |
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| _version_ | 1864513437190586368 |
|---|---|
| author | Balaha, Farah |
| author2 | Alhosani, Maryam Asa'd, Randa Chillingarian, Igor V. |
| author2_role | author author author |
| author_facet | Balaha, Farah Alhosani, Maryam Asa'd, Randa Chillingarian, Igor V. |
| author_role | author |
| dc.creator.none.fl_str_mv | Balaha, Farah Alhosani, Maryam Asa'd, Randa Chillingarian, Igor V. |
| dc.date.none.fl_str_mv | 2019 2020-02-19T09:07:16Z 2020-02-19T09:07:16Z |
| dc.format.none.fl_str_mv | application/pdf |
| dc.identifier.none.fl_str_mv | Farah Balaha et al 2019 J. Phys.: Conf. Ser. 1258 012020 1742-6596 http://hdl.handle.net/11073/16614 10.1088/1742-6596/1258/1/012020 |
| dc.language.none.fl_str_mv | en_US |
| dc.publisher.none.fl_str_mv | IOP Science |
| dc.relation.none.fl_str_mv | https://doi.org/10.1088/1742-6596/1258/1/012020 |
| dc.title.none.fl_str_mv | Using the Age and Metallicity of 8 Star Clusters to confirm the Chemical Enrichment History of the LMC |
| dc.type.none.fl_str_mv | Peer-Reviewed Published version info:eu-repo/semantics/publishedVersion info:eu-repo/semantics/article |
| description | In this paper, we find the ages and metallicities of 8 Large Magellanic Cloud (LMC) star clusters obtained from integrated light spectra and use them to obtain the Chemical Enrichment History of the host galaxy. Our results are in good agreement with those obtained from resolved studies. This confirms that this method can be used for far away galaxies for which their star clusters are not resolved. |
| format | article |
| id | aus_690cff79975062d604ed82dc548371e8 |
| identifier_str_mv | Farah Balaha et al 2019 J. Phys.: Conf. Ser. 1258 012020 1742-6596 10.1088/1742-6596/1258/1/012020 |
| language_invalid_str_mv | en_US |
| network_acronym_str | aus |
| network_name_str | aus |
| oai_identifier_str | oai:repository.aus.edu:11073/16614 |
| publishDate | 2019 |
| publisher.none.fl_str_mv | IOP Science |
| repository.mail.fl_str_mv | |
| repository.name.fl_str_mv | |
| repository_id_str | |
| spelling | Using the Age and Metallicity of 8 Star Clusters to confirm the Chemical Enrichment History of the LMCBalaha, FarahAlhosani, MaryamAsa'd, RandaChillingarian, Igor V.In this paper, we find the ages and metallicities of 8 Large Magellanic Cloud (LMC) star clusters obtained from integrated light spectra and use them to obtain the Chemical Enrichment History of the host galaxy. Our results are in good agreement with those obtained from resolved studies. This confirms that this method can be used for far away galaxies for which their star clusters are not resolved.IOP Science2020-02-19T09:07:16Z2020-02-19T09:07:16Z2019Peer-ReviewedPublished versioninfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articleapplication/pdfFarah Balaha et al 2019 J. Phys.: Conf. Ser. 1258 0120201742-6596http://hdl.handle.net/11073/1661410.1088/1742-6596/1258/1/012020en_UShttps://doi.org/10.1088/1742-6596/1258/1/012020oai:repository.aus.edu:11073/166142024-08-22T12:02:29Z |
| spellingShingle | Using the Age and Metallicity of 8 Star Clusters to confirm the Chemical Enrichment History of the LMC Balaha, Farah |
| status_str | publishedVersion |
| title | Using the Age and Metallicity of 8 Star Clusters to confirm the Chemical Enrichment History of the LMC |
| title_full | Using the Age and Metallicity of 8 Star Clusters to confirm the Chemical Enrichment History of the LMC |
| title_fullStr | Using the Age and Metallicity of 8 Star Clusters to confirm the Chemical Enrichment History of the LMC |
| title_full_unstemmed | Using the Age and Metallicity of 8 Star Clusters to confirm the Chemical Enrichment History of the LMC |
| title_short | Using the Age and Metallicity of 8 Star Clusters to confirm the Chemical Enrichment History of the LMC |
| title_sort | Using the Age and Metallicity of 8 Star Clusters to confirm the Chemical Enrichment History of the LMC |
| url | http://hdl.handle.net/11073/16614 |