Deep imaging of Virgo Z : not a nearby ultrafaint dwarf galaxy, but a distant compact group of galaxies
Context. The search for Milky Way faint satellite galaxies and star clusters has been intensified in recent years thanks to the Sloan Digital Sky Survey (SDSS), and other efforts to verify candidate objects. Aims. We observed the Milky Way satellite candidate Vir Z, reported by Walsh et al. (2009, A...
| Autores: | , , , |
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| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2013 |
| País: | Brasil |
| Institución: | Universidade Federal do Rio Grande do Sul (UFRGS) |
| Repositorio: | Repositório Institucional da UFRGS |
| Idioma: | inglés |
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| Acceso en línea: | http://hdl.handle.net/10183/109478 |
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| Palabra clave: | Aglomerados de galaxias Galaxia Galaxy: general Galaxies: groups: individual: Virgo Z |
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2015-01-30T02:18:03Z20130004-6361http://hdl.handle.net/10183/109478000948907Context. The search for Milky Way faint satellite galaxies and star clusters has been intensified in recent years thanks to the Sloan Digital Sky Survey (SDSS), and other efforts to verify candidate objects. Aims. We observed the Milky Way satellite candidate Vir Z, reported by Walsh et al. (2009, AJ, 137, 450), from the detection of an overdensity in the SDSS database. Methods. Deep subarcsec seeing images from the New Technology Telescope (NTT) and Galileo telescopes were obtained in order to infer the nature of the proposed overdensity. Results. The image and colour-magnitude diagram of the Vir Z field shows no dwarf galaxy. Instead, we identified a compact group of galaxies near the center of the Vir Z field at redshift z ≈ 0.3 ± 0.2, based on the apparent magnitudes of the brightest galaxies assuming L = L∗, and on angular sizes of the spirals assuming physical sizes equal to M31.application/pdfengAstronomy and astrophysics. Les Ulis. Vol. 559 (Nov. 2013), A61, 4 p.Aglomerados de galaxiasGalaxiaGalaxy: generalGalaxies: groups: individual: Virgo ZDeep imaging of Virgo Z : not a nearby ultrafaint dwarf galaxy, but a distant compact group of galaxiesEstrangeiroinfo: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:UFRGSBarbuy, BeatrizBica, Eduardo Luiz DamianiOrtolani, SergioSouza, André Lopes deORIGINAL000948907.pdf000948907.pdfTexto completo (inglês)application/pdf314506http://www.lume.ufrgs.br/bitstream/10183/109478/1/000948907.pdf6a3c0c4270e4beb644baa44b19d765a1MD51TEXT000948907.pdf.txt000948907.pdf.txtExtracted Texttext/plain19574http://www.lume.ufrgs.br/bitstream/10183/109478/2/000948907.pdf.txt5142b581992834c2085da0fdaf7acf90MD52THUMBNAIL000948907.pdf.jpg000948907.pdf.jpgGenerated Thumbnailimage/jpeg2023http://www.lume.ufrgs.br/bitstream/10183/109478/3/000948907.pdf.jpg0b9f6600817815f5e19569cea708d3a2MD5310183/1094782023-10-25 03:38:58.600462oai:www.lume.ufrgs.br:10183/109478Repositório InstitucionalPUBhttps://lume.ufrgs.br/oai/requestlume@ufrgs.bropendoar:2023-10-25T06:38:58Repositório Institucional da UFRGS - Universidade Federal do Rio Grande do Sul (UFRGS)false |
| dc.title.pt_BR.fl_str_mv |
Deep imaging of Virgo Z : not a nearby ultrafaint dwarf galaxy, but a distant compact group of galaxies |
| title |
Deep imaging of Virgo Z : not a nearby ultrafaint dwarf galaxy, but a distant compact group of galaxies |
| spellingShingle |
Deep imaging of Virgo Z : not a nearby ultrafaint dwarf galaxy, but a distant compact group of galaxies Barbuy, Beatriz Aglomerados de galaxias Galaxia Galaxy: general Galaxies: groups: individual: Virgo Z |
| title_short |
Deep imaging of Virgo Z : not a nearby ultrafaint dwarf galaxy, but a distant compact group of galaxies |
| title_full |
Deep imaging of Virgo Z : not a nearby ultrafaint dwarf galaxy, but a distant compact group of galaxies |
| title_fullStr |
Deep imaging of Virgo Z : not a nearby ultrafaint dwarf galaxy, but a distant compact group of galaxies |
| title_full_unstemmed |
Deep imaging of Virgo Z : not a nearby ultrafaint dwarf galaxy, but a distant compact group of galaxies |
| title_sort |
Deep imaging of Virgo Z : not a nearby ultrafaint dwarf galaxy, but a distant compact group of galaxies |
| dc.creator.none.fl_str_mv |
Barbuy, Beatriz Bica, Eduardo Luiz Damiani Ortolani, Sergio Souza, André Lopes de |
| author |
Barbuy, Beatriz |
| author_facet |
Barbuy, Beatriz Bica, Eduardo Luiz Damiani Ortolani, Sergio Souza, André Lopes de |
| author_role |
author |
| author2 |
Bica, Eduardo Luiz Damiani Ortolani, Sergio Souza, André Lopes de |
| author2_role |
author author author |
| dc.subject.por.fl_str_mv |
Aglomerados de galaxias Galaxia |
| topic |
Aglomerados de galaxias Galaxia Galaxy: general Galaxies: groups: individual: Virgo Z |
| dc.subject.eng.fl_str_mv |
Galaxy: general Galaxies: groups: individual: Virgo Z |
| description |
Context. The search for Milky Way faint satellite galaxies and star clusters has been intensified in recent years thanks to the Sloan Digital Sky Survey (SDSS), and other efforts to verify candidate objects. Aims. We observed the Milky Way satellite candidate Vir Z, reported by Walsh et al. (2009, AJ, 137, 450), from the detection of an overdensity in the SDSS database. Methods. Deep subarcsec seeing images from the New Technology Telescope (NTT) and Galileo telescopes were obtained in order to infer the nature of the proposed overdensity. Results. The image and colour-magnitude diagram of the Vir Z field shows no dwarf galaxy. Instead, we identified a compact group of galaxies near the center of the Vir Z field at redshift z ≈ 0.3 ± 0.2, based on the apparent magnitudes of the brightest galaxies assuming L = L∗, and on angular sizes of the spirals assuming physical sizes equal to M31. |
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2013 |
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2013 |
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2015-01-30T02:18:03Z |
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Estrangeiro info:eu-repo/semantics/article |
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http://hdl.handle.net/10183/109478 |
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0004-6361 |
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000948907 |
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eng |
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Astronomy and astrophysics. Les Ulis. Vol. 559 (Nov. 2013), A61, 4 p. |
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