Colour-magnitude diagrams of the inner halo globular clusters NGC 5986 and NGC 6712
Autor(a) principal: | |
---|---|
Data de Publicação: | 2000 |
Outros Autores: | , , , |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UFRGS |
Texto Completo: | http://hdl.handle.net/10183/98511 |
Resumo: | We present V and I photometry for NGC 5986 and B and V for NGC 6712. NGC 5986 has a blue extended horizontal branch, while NGC 6712 has a composite red and blue horizontal branch, where the latter extends to unusual bluer colours. Both clusters have RR Lyrae. We derive a reddening E(B-V) ≈ 0.29 and a distance from the Sun dʘ ≈ 11.2 kpc for NGC 5986, and E(B-V) ≈ 0.33 and dʘ ≈ 7.9 kpc for NGC 6712. Their galactocentric distances of RGC = 5.2 and 3.6 kpc respectively, locate them in the inner halo; NGC 6712 could be considered to be located in the bulge. NGC 6712 has |z|≈ 500 pc, indicating that the cluster is crossing the disk. We estimate metallicities of [Fe/H] = -1.6 and -1.0 respectively for NGC 5986 and NGC 6712. |
id |
UFRGS-2_c80a74a857e6723f48201b7f0ea58ec6 |
---|---|
oai_identifier_str |
oai:www.lume.ufrgs.br:10183/98511 |
network_acronym_str |
UFRGS-2 |
network_name_str |
Repositório Institucional da UFRGS |
repository_id_str |
|
spelling |
Ortolani, SergioMomany, YazanBarbuy, BeatrizBica, Eduardo Luiz DamianiCatelan, Márcio2014-07-24T02:04:22Z20000004-6361http://hdl.handle.net/10183/98511000279544We present V and I photometry for NGC 5986 and B and V for NGC 6712. NGC 5986 has a blue extended horizontal branch, while NGC 6712 has a composite red and blue horizontal branch, where the latter extends to unusual bluer colours. Both clusters have RR Lyrae. We derive a reddening E(B-V) ≈ 0.29 and a distance from the Sun dʘ ≈ 11.2 kpc for NGC 5986, and E(B-V) ≈ 0.33 and dʘ ≈ 7.9 kpc for NGC 6712. Their galactocentric distances of RGC = 5.2 and 3.6 kpc respectively, locate them in the inner halo; NGC 6712 could be considered to be located in the bulge. NGC 6712 has |z|≈ 500 pc, indicating that the cluster is crossing the disk. We estimate metallicities of [Fe/H] = -1.6 and -1.0 respectively for NGC 5986 and NGC 6712.application/pdfengAstronomy and astrophysics. New York. Vol. 362, no. 3 (Oct. 2000), p. 953-958AstronomiaStars: Hertzsprung–Russell (HR) and C-M diagramsGalaxy: globular clusters: individual: NGC 5986, NGC 6712Colour-magnitude diagrams of the inner halo globular clusters NGC 5986 and NGC 6712Estrangeiroinfo: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:UFRGSORIGINAL000279544.pdf000279544.pdfTexto completo (inglês)application/pdf746097http://www.lume.ufrgs.br/bitstream/10183/98511/1/000279544.pdf04e0d0b7881a27220d19a4851adb1e66MD51TEXT000279544.pdf.txt000279544.pdf.txtExtracted Texttext/plain23218http://www.lume.ufrgs.br/bitstream/10183/98511/2/000279544.pdf.txt24c29fc0f546678f5c1d979fd6b404a7MD52THUMBNAIL000279544.pdf.jpg000279544.pdf.jpgGenerated Thumbnailimage/jpeg2053http://www.lume.ufrgs.br/bitstream/10183/98511/3/000279544.pdf.jpg99aff9bcbe5e96fa7963297fec573aebMD5310183/985112024-04-13 06:45:54.244475oai:www.lume.ufrgs.br:10183/98511Repositório de PublicaçõesPUBhttps://lume.ufrgs.br/oai/requestopendoar:2024-04-13T09:45:54Repositório Institucional da UFRGS - Universidade Federal do Rio Grande do Sul (UFRGS)false |
dc.title.pt_BR.fl_str_mv |
Colour-magnitude diagrams of the inner halo globular clusters NGC 5986 and NGC 6712 |
title |
Colour-magnitude diagrams of the inner halo globular clusters NGC 5986 and NGC 6712 |
spellingShingle |
Colour-magnitude diagrams of the inner halo globular clusters NGC 5986 and NGC 6712 Ortolani, Sergio Astronomia Stars: Hertzsprung–Russell (HR) and C-M diagrams Galaxy: globular clusters: individual: NGC 5986, NGC 6712 |
title_short |
Colour-magnitude diagrams of the inner halo globular clusters NGC 5986 and NGC 6712 |
title_full |
Colour-magnitude diagrams of the inner halo globular clusters NGC 5986 and NGC 6712 |
title_fullStr |
Colour-magnitude diagrams of the inner halo globular clusters NGC 5986 and NGC 6712 |
title_full_unstemmed |
Colour-magnitude diagrams of the inner halo globular clusters NGC 5986 and NGC 6712 |
title_sort |
Colour-magnitude diagrams of the inner halo globular clusters NGC 5986 and NGC 6712 |
author |
Ortolani, Sergio |
author_facet |
Ortolani, Sergio Momany, Yazan Barbuy, Beatriz Bica, Eduardo Luiz Damiani Catelan, Márcio |
author_role |
author |
author2 |
Momany, Yazan Barbuy, Beatriz Bica, Eduardo Luiz Damiani Catelan, Márcio |
author2_role |
author author author author |
dc.contributor.author.fl_str_mv |
Ortolani, Sergio Momany, Yazan Barbuy, Beatriz Bica, Eduardo Luiz Damiani Catelan, Márcio |
dc.subject.por.fl_str_mv |
Astronomia |
topic |
Astronomia Stars: Hertzsprung–Russell (HR) and C-M diagrams Galaxy: globular clusters: individual: NGC 5986, NGC 6712 |
dc.subject.eng.fl_str_mv |
Stars: Hertzsprung–Russell (HR) and C-M diagrams Galaxy: globular clusters: individual: NGC 5986, NGC 6712 |
description |
We present V and I photometry for NGC 5986 and B and V for NGC 6712. NGC 5986 has a blue extended horizontal branch, while NGC 6712 has a composite red and blue horizontal branch, where the latter extends to unusual bluer colours. Both clusters have RR Lyrae. We derive a reddening E(B-V) ≈ 0.29 and a distance from the Sun dʘ ≈ 11.2 kpc for NGC 5986, and E(B-V) ≈ 0.33 and dʘ ≈ 7.9 kpc for NGC 6712. Their galactocentric distances of RGC = 5.2 and 3.6 kpc respectively, locate them in the inner halo; NGC 6712 could be considered to be located in the bulge. NGC 6712 has |z|≈ 500 pc, indicating that the cluster is crossing the disk. We estimate metallicities of [Fe/H] = -1.6 and -1.0 respectively for NGC 5986 and NGC 6712. |
publishDate |
2000 |
dc.date.issued.fl_str_mv |
2000 |
dc.date.accessioned.fl_str_mv |
2014-07-24T02:04:22Z |
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/10183/98511 |
dc.identifier.issn.pt_BR.fl_str_mv |
0004-6361 |
dc.identifier.nrb.pt_BR.fl_str_mv |
000279544 |
identifier_str_mv |
0004-6361 000279544 |
url |
http://hdl.handle.net/10183/98511 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.ispartof.pt_BR.fl_str_mv |
Astronomy and astrophysics. New York. Vol. 362, no. 3 (Oct. 2000), p. 953-958 |
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 |
instname_str |
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/10183/98511/1/000279544.pdf http://www.lume.ufrgs.br/bitstream/10183/98511/2/000279544.pdf.txt http://www.lume.ufrgs.br/bitstream/10183/98511/3/000279544.pdf.jpg |
bitstream.checksum.fl_str_mv |
04e0d0b7881a27220d19a4851adb1e66 24c29fc0f546678f5c1d979fd6b404a7 99aff9bcbe5e96fa7963297fec573aeb |
bitstream.checksumAlgorithm.fl_str_mv |
MD5 MD5 MD5 |
repository.name.fl_str_mv |
Repositório Institucional da UFRGS - Universidade Federal do Rio Grande do Sul (UFRGS) |
repository.mail.fl_str_mv |
|
_version_ |
1815447550525702144 |