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Discovery of the first wide L dwarf plus giant binary system and eight other ultracool dwarfs in wide binaries

文献类型:期刊论文

作者Zhang, ZH1; Pinfield, DJ1; Day-Jones, AC1,2; Burningham, B1; Jones, HRA1; Yu, S3; Jenkins, JS2; Han ZW(韩占文)4,5; Galvez-Ortiz, MC1; Gallardo, J2
刊名MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
出版日期2010-06-01
卷号404期号:4页码:1817-1834
关键词binaries: general brown dwarfs stars: individual: eta Cancri stars: late-type stars: low-mass
ISSN号0035-8711
产权排序第四完成单位
通讯作者Zhang, ZH (reprint author), Univ Hertfordshire, Sci & Technol Res Inst, Ctr Astrophys Res, Hatfield AL10 9AB, Herts, England.
英文摘要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 eta Cancri. Such primaries can provide age and metallicity constraints for any companion objects, yielding excellent benchmark objects. eta Cancri AB is the first wide ultracool dwarf + giant binary system identified. We present new observations and analysis that constrain the metallicity of eta 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 eta Cancri B is a single object, we estimate its physical attributes to be mass = 63-82 M(Jup), T(eff) = 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 eta 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.
WOS标题词Science & Technology ; Physical Sciences
学科主题Astronomy & Astrophysics
类目[WOS]Astronomy & Astrophysics
研究领域[WOS]Astronomy & Astrophysics
关键词[WOS]DIGITAL SKY SURVEY ; STAR ADAPTIVE OPTICS ; LOW-MASS STARS ; PROPER-MOTION CATALOG ; BROWN DWARF ; T-DWARF ; DATA RELEASE ; SUBSTELLAR COMPANION ; NEARBY STARS ; SOLAR NEIGHBORHOOD
收录类别SCI
原文出处http://mnras.oxfordjournals.org/content/404/4/1817
语种英语
WOS记录号WOS:000277981400014
源URL[http://ir.ynao.ac.cn/handle/114a53/4501]  
专题云南天文台_大样本恒星演化研究组
云南天文台_中国科学院天体结构与演化重点实验室
作者单位1.Centre for Astrophysics Research, Science and Technology Research Institute, University of Hertfordshrie, Hatfield AL10 9AB
2.Department of Astronomy, Universidad de Chile, Casilla Postal 36D, Santiago, Chile
3.Armagh Observatory, College Hill, Armagh BT61 9DG
4.National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, Kunming 650011, China
5.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences
6.Department of Astronomy, University of Virginia, PO Box 400325, Charlottesville, VA 22904-4325, USA
7.School of Physics, University of New South Wales, NSW 2050, Australia
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GB/T 7714
Zhang, ZH,Pinfield, DJ,Day-Jones, AC,et al. Discovery of the first wide L dwarf plus giant binary system and eight other ultracool dwarfs in wide binaries[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2010,404(4):1817-1834.
APA Zhang, ZH.,Pinfield, DJ.,Day-Jones, AC.,Burningham, B.,Jones, HRA.,...&R. S. Pokorny.(2010).Discovery of the first wide L dwarf plus giant binary system and eight other ultracool dwarfs in wide binaries.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,404(4),1817-1834.
MLA Zhang, ZH,et al."Discovery of the first wide L dwarf plus giant binary system and eight other ultracool dwarfs in wide binaries".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 404.4(2010):1817-1834.

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