Discovery of the first wide L dwarf + giant binary system and eight other ultracool dwarfs in wide binaries
We identify 806 ultracool dwarfs (of which 34 are newly discovered L dwarfs) from their Sloan Digital Sky Survey (SDSS) riz photometry and obtain proper motions through cross-matching with the United Kingdom Infrared Telescope Infrared Deep Sky Survey (UKIDSS) and Two-Micron All-Sky Survey (2MASS)....
| Autores: | , , , , , , , , , , , , , |
|---|---|
| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2010 |
| País: | Chile |
| Idioma: | inglés |
| OAI Identifier: | oai:repositorio.anid.cl:10533/245882 |
| Acceso en línea: | https://hdl.handle.net/10533/245882 |
| Access Level: | acceso abierto |
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Pokorny, R. S.Tinney, C. G.Weights, D.García-Pérez, A. E.Gallardo, J.Gálvez-Ortiz, M. C.Han, Z.Jenkins, J. S.Yu, S.Jones, H. R. A.Burningham, B.Day-Jones, A. C.Pinfield, D. J.Zhang, Z. H.2010 10.1111/j.1365-2966.2010.16394.xhttps://hdl.handle.net/10533/245882http://purl.org/coar/access_right/c_abf2Discovery of the first wide L dwarf + giant binary system and eight other ultracool dwarfs in wide binariesZhang, Z. H.Pinfield, D. J.Day-Jones, A. C.Burningham, B.Jones, H. R. A.Yu, S.Jenkins, J. S.Han, Z.Gálvez-Ortiz, M. C.Gallardo, J.García-Pérez, A. E.Weights, D.Tinney, C. G.Pokorny, R. S.2020-08-14T20:42:47Z2022-07-08T20:15:51Z2020-08-14T20:42:47Z2022-07-08T20:15:51Z2010We identify 806 ultracool dwarfs (of which 34 are newly discovered L dwarfs) from their Sloan Digital Sky Survey (SDSS) riz photometry and obtain proper motions through cross-matching with the United Kingdom Infrared Telescope Infrared Deep Sky Survey (UKIDSS) and Two-Micron All-Sky Survey (2MASS). Proper-motion and distance constraints show that nine of our ultracool dwarfs are members of widely separated binary systems: SDSS 0101 (K5V+M9.5V), SDSS 0207 (M1.5V+L3V), SDSS 0832 (K3III+L3.5V), SDSS 0858 (M4V+L0V), SDSS 0953 (M4V+M9.5V), SDSS 0956 (M2V+M9V), SDSS 1304 (M4.5V+L0V), SDSS 1631 (M5.5V+M8V) and SDSS 1638 (M4V+L0V). One of these (SDSS 0832) is shown to be a companion to the bright K3 giant η Cancri. Such primaries can provide age and metallicity constraints for any companion objects, yielding excellent benchmark objects. η Cancri AB is the first wide ultracool dwarf + giant binary system identified. We present new observations and analysis that constrain the metallicity of η Cancri A to be near-solar, and use recent evolutionary models to constrain the age of the giant to be 2.2–6.1 Gyr. If η Cancri B is a single object, we estimate its physical attributes to be mass = 63–82 MJup, Teff= 1800 ± 150 K, log g= 5.3–5.5, [M/H]= 0.0 ± 0.1. Its colours are non-typical when compared with other ultracool dwarfs, and we also assess the possibility that η Cancri B is itself an unresolved binary, showing that the combined light of an L4 + T4 system could provide a reasonable explanation for its colours.CENASTROFONDAPFONDAP1501000315010003virtual::46653-1WOS:000277981400014https://hdl.handle.net/10533/245882enginstname: ANIDreponame: Repositorio Digital RI2.0 10.1111/j.1365-2966.2010.16394.xhttps://academic.oup.com/mnras/article/404/4/1817/1082602info:eu-repo/semantics/openAccessDiscovery of the first wide L dwarf + giant binary system and eight other ultracool dwarfs in wide binariesMonthly Notices of the Royal Astronomical SocietyArticuloinfo:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttps://hdl.handle.net/10533/245882FONDAPhttp://purl.org/coar/resource_type/c_2df8fbb1045fc0e1-ef55-4532-8afe-69fe789d964dvirtual::46653-1045fc0e1-ef55-4532-8afe-69fe789d964dvirtual::46653-110533/245882oai:repositorio.anid.cl:10533/2458822023-07-24 17:58:41.951https://repositorio.anid.clRepositorio ANIDaletelier@anid.cl |
| dc.title.none.fl_str_mv |
Discovery of the first wide L dwarf + giant binary system and eight other ultracool dwarfs in wide binaries |
| dc.title.journal.none.fl_str_mv |
Monthly Notices of the Royal Astronomical Society |
| title |
Discovery of the first wide L dwarf + giant binary system and eight other ultracool dwarfs in wide binaries |
| spellingShingle |
Discovery of the first wide L dwarf + giant binary system and eight other ultracool dwarfs in wide binaries Zhang, Z. H. |
| title_short |
Discovery of the first wide L dwarf + giant binary system and eight other ultracool dwarfs in wide binaries |
| title_full |
Discovery of the first wide L dwarf + giant binary system and eight other ultracool dwarfs in wide binaries |
| title_fullStr |
Discovery of the first wide L dwarf + giant binary system and eight other ultracool dwarfs in wide binaries |
| title_full_unstemmed |
Discovery of the first wide L dwarf + giant binary system and eight other ultracool dwarfs in wide binaries |
| title_sort |
Discovery of the first wide L dwarf + giant binary system and eight other ultracool dwarfs in wide binaries |
| dc.creator.none.fl_str_mv |
Zhang, Z. H. Pinfield, D. J. Day-Jones, A. C. Burningham, B. Jones, H. R. A. Yu, S. Jenkins, J. S. Han, Z. Gálvez-Ortiz, M. C. Gallardo, J. García-Pérez, A. E. Weights, D. Tinney, C. G. Pokorny, R. S. |
| author |
Zhang, Z. H. |
| author_facet |
Zhang, Z. H. Pinfield, D. J. Day-Jones, A. C. Burningham, B. Jones, H. R. A. Yu, S. Jenkins, J. S. Han, Z. Gálvez-Ortiz, M. C. Gallardo, J. García-Pérez, A. E. Weights, D. Tinney, C. G. Pokorny, R. S. |
| author_role |
author |
| author2 |
Pinfield, D. J. Day-Jones, A. C. Burningham, B. Jones, H. R. A. Yu, S. Jenkins, J. S. Han, Z. Gálvez-Ortiz, M. C. Gallardo, J. García-Pérez, A. E. Weights, D. Tinney, C. G. Pokorny, R. S. |
| author2_role |
author author author author author author author author author author author author author |
| description |
We identify 806 ultracool dwarfs (of which 34 are newly discovered L dwarfs) from their Sloan Digital Sky Survey (SDSS) riz photometry and obtain proper motions through cross-matching with the United Kingdom Infrared Telescope Infrared Deep Sky Survey (UKIDSS) and Two-Micron All-Sky Survey (2MASS). Proper-motion and distance constraints show that nine of our ultracool dwarfs are members of widely separated binary systems: SDSS 0101 (K5V+M9.5V), SDSS 0207 (M1.5V+L3V), SDSS 0832 (K3III+L3.5V), SDSS 0858 (M4V+L0V), SDSS 0953 (M4V+M9.5V), SDSS 0956 (M2V+M9V), SDSS 1304 (M4.5V+L0V), SDSS 1631 (M5.5V+M8V) and SDSS 1638 (M4V+L0V). One of these (SDSS 0832) is shown to be a companion to the bright K3 giant η Cancri. Such primaries can provide age and metallicity constraints for any companion objects, yielding excellent benchmark objects. η Cancri AB is the first wide ultracool dwarf + giant binary system identified. We present new observations and analysis that constrain the metallicity of η Cancri A to be near-solar, and use recent evolutionary models to constrain the age of the giant to be 2.2–6.1 Gyr. If η Cancri B is a single object, we estimate its physical attributes to be mass = 63–82 MJup, Teff= 1800 ± 150 K, log g= 5.3–5.5, [M/H]= 0.0 ± 0.1. Its colours are non-typical when compared with other ultracool dwarfs, and we also assess the possibility that η Cancri B is itself an unresolved binary, showing that the combined light of an L4 + T4 system could provide a reasonable explanation for its colours. |
| publishDate |
2010 |
| dc.date.issued.none.fl_str_mv |
2010 |
| dc.date.accessioned.none.fl_str_mv |
2020-08-14T20:42:47Z 2022-07-08T20:15:51Z |
| dc.date.available.none.fl_str_mv |
2020-08-14T20:42:47Z 2022-07-08T20:15:51Z |
| dc.type.none.fl_str_mv |
Articulo |
| dc.type.driver.none.fl_str_mv |
info:eu-repo/semantics/article |
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info:eu-repo/semantics/publishedVersion |
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article |
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publishedVersion |
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15010003 15010003 |
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WOS:000277981400014 |
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https://hdl.handle.net/10533/245882 |
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15010003 WOS:000277981400014 |
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https://hdl.handle.net/10533/245882 |
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eng |
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eng |
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instname: ANID reponame: Repositorio Digital RI2.0 |
| dc.relation.doi.none.fl_str_mv |
10.1111/j.1365-2966.2010.16394.x |
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https://academic.oup.com/mnras/article/404/4/1817/1082602 |
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info:eu-repo/semantics/openAccess |
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openAccess |
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Repositorio ANID |
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aletelier@anid.cl |
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