Gemini-Phoenix infrared high-resolution abundance analysis of five giants in the bulge globular cluster NGC 6553
Autor(a) principal: | |
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Data de Publicação: | 2003 |
Outros Autores: | , , , , , |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UFRGS |
Texto Completo: | http://hdl.handle.net/10183/206328 |
Resumo: | A detailed abundance analysis of 5 giants of the metal-rich bulge globular cluster NGC 6553 was carried out using high resolution infrared spectra in the H band, obtained at the Gemini-South 8m telescope. JK photometry collected at ESO and VI photometry from the Hubble Space Telescope are used to derive effective temperatures. The present analysis provides a metallicity [Fe/H] = -0.20±0.10. An overabundance of oxygen of [O/Fe] = +0.20 is found from IR OH lines. |
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Meléndez, JorgeBarbuy, BeatrizBica, Eduardo Luiz DamianiZoccali, ManuelaOrtolani, SergioRenzini, AlvioHill, Vanessa2020-02-28T04:07:03Z20030004-6361http://hdl.handle.net/10183/206328000391528A detailed abundance analysis of 5 giants of the metal-rich bulge globular cluster NGC 6553 was carried out using high resolution infrared spectra in the H band, obtained at the Gemini-South 8m telescope. JK photometry collected at ESO and VI photometry from the Hubble Space Telescope are used to derive effective temperatures. The present analysis provides a metallicity [Fe/H] = -0.20±0.10. An overabundance of oxygen of [O/Fe] = +0.20 is found from IR OH lines.
application/pdfengAstronomy and astrophysics. Les Ulis. Vol. 411, no. 3 (Dec. 2003), p. 417-426Semicondutores elementaresGermânioImplantacao ionicaNanopartículasOxidaçãoTamanho de partículaFotoluminescênciaRetroespalhamento rutherfordCompostos de silícioMicroscopia eletrônica de transmissãoEspectros ultravioletaStars: abundances, atmospheresGalaxy: globular clusters: individual: NGC 6553Gemini-Phoenix infrared high-resolution abundance analysis of five giants in the bulge globular cluster NGC 6553Estrangeiroinfo:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/openAccessreponame:Repositório Institucional da UFRGSinstname:Universidade Federal do Rio Grande do Sul (UFRGS)instacron:UFRGSTEXT000391528.pdf.txt000391528.pdf.txtExtracted Texttext/plain34931http://www.lume.ufrgs.br/bitstream/10183/206328/2/000391528.pdf.txt347681abceb27a43fbde717b037eedefMD52ORIGINAL000391528.pdfTexto completo (inglês)application/pdf1328578http://www.lume.ufrgs.br/bitstream/10183/206328/1/000391528.pdf91a151e498fba671e0acd983af59eea4MD5110183/2063282024-04-12 06:20:36.096964oai:www.lume.ufrgs.br:10183/206328Repositório de PublicaçõesPUBhttps://lume.ufrgs.br/oai/requestopendoar:2024-04-12T09:20:36Repositório Institucional da UFRGS - Universidade Federal do Rio Grande do Sul (UFRGS)false |
dc.title.pt_BR.fl_str_mv |
Gemini-Phoenix infrared high-resolution abundance analysis of five giants in the bulge globular cluster NGC 6553 |
title |
Gemini-Phoenix infrared high-resolution abundance analysis of five giants in the bulge globular cluster NGC 6553 |
spellingShingle |
Gemini-Phoenix infrared high-resolution abundance analysis of five giants in the bulge globular cluster NGC 6553 Meléndez, Jorge Semicondutores elementares Germânio Implantacao ionica Nanopartículas Oxidação Tamanho de partícula Fotoluminescência Retroespalhamento rutherford Compostos de silício Microscopia eletrônica de transmissão Espectros ultravioleta Stars: abundances, atmospheres Galaxy: globular clusters: individual: NGC 6553 |
title_short |
Gemini-Phoenix infrared high-resolution abundance analysis of five giants in the bulge globular cluster NGC 6553 |
title_full |
Gemini-Phoenix infrared high-resolution abundance analysis of five giants in the bulge globular cluster NGC 6553 |
title_fullStr |
Gemini-Phoenix infrared high-resolution abundance analysis of five giants in the bulge globular cluster NGC 6553 |
title_full_unstemmed |
Gemini-Phoenix infrared high-resolution abundance analysis of five giants in the bulge globular cluster NGC 6553 |
title_sort |
Gemini-Phoenix infrared high-resolution abundance analysis of five giants in the bulge globular cluster NGC 6553 |
author |
Meléndez, Jorge |
author_facet |
Meléndez, Jorge Barbuy, Beatriz Bica, Eduardo Luiz Damiani Zoccali, Manuela Ortolani, Sergio Renzini, Alvio Hill, Vanessa |
author_role |
author |
author2 |
Barbuy, Beatriz Bica, Eduardo Luiz Damiani Zoccali, Manuela Ortolani, Sergio Renzini, Alvio Hill, Vanessa |
author2_role |
author author author author author author |
dc.contributor.author.fl_str_mv |
Meléndez, Jorge Barbuy, Beatriz Bica, Eduardo Luiz Damiani Zoccali, Manuela Ortolani, Sergio Renzini, Alvio Hill, Vanessa |
dc.subject.por.fl_str_mv |
Semicondutores elementares Germânio Implantacao ionica Nanopartículas Oxidação Tamanho de partícula Fotoluminescência Retroespalhamento rutherford Compostos de silício Microscopia eletrônica de transmissão Espectros ultravioleta |
topic |
Semicondutores elementares Germânio Implantacao ionica Nanopartículas Oxidação Tamanho de partícula Fotoluminescência Retroespalhamento rutherford Compostos de silício Microscopia eletrônica de transmissão Espectros ultravioleta Stars: abundances, atmospheres Galaxy: globular clusters: individual: NGC 6553 |
dc.subject.eng.fl_str_mv |
Stars: abundances, atmospheres Galaxy: globular clusters: individual: NGC 6553 |
description |
A detailed abundance analysis of 5 giants of the metal-rich bulge globular cluster NGC 6553 was carried out using high resolution infrared spectra in the H band, obtained at the Gemini-South 8m telescope. JK photometry collected at ESO and VI photometry from the Hubble Space Telescope are used to derive effective temperatures. The present analysis provides a metallicity [Fe/H] = -0.20±0.10. An overabundance of oxygen of [O/Fe] = +0.20 is found from IR OH lines.
|
publishDate |
2003 |
dc.date.issued.fl_str_mv |
2003 |
dc.date.accessioned.fl_str_mv |
2020-02-28T04:07:03Z |
dc.type.driver.fl_str_mv |
Estrangeiro info:eu-repo/semantics/article |
dc.type.status.fl_str_mv |
info:eu-repo/semantics/publishedVersion |
format |
article |
status_str |
publishedVersion |
dc.identifier.uri.fl_str_mv |
http://hdl.handle.net/10183/206328 |
dc.identifier.issn.pt_BR.fl_str_mv |
0004-6361 |
dc.identifier.nrb.pt_BR.fl_str_mv |
000391528 |
identifier_str_mv |
0004-6361 000391528 |
url |
http://hdl.handle.net/10183/206328 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.ispartof.pt_BR.fl_str_mv |
Astronomy and astrophysics. Les Ulis. Vol. 411, no. 3 (Dec. 2003), p. 417-426 |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
dc.format.none.fl_str_mv |
application/pdf |
dc.source.none.fl_str_mv |
reponame:Repositório Institucional da UFRGS instname:Universidade Federal do Rio Grande do Sul (UFRGS) instacron:UFRGS |
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Universidade Federal do Rio Grande do Sul (UFRGS) |
instacron_str |
UFRGS |
institution |
UFRGS |
reponame_str |
Repositório Institucional da UFRGS |
collection |
Repositório Institucional da UFRGS |
bitstream.url.fl_str_mv |
http://www.lume.ufrgs.br/bitstream/10183/206328/2/000391528.pdf.txt http://www.lume.ufrgs.br/bitstream/10183/206328/1/000391528.pdf |
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