The intermediate-age brown dwarf LP 944-20

被引:89
作者
Tinney, CG [1 ]
机构
[1] Anglo Australian Observ, Epping, NSW 2121, Australia
关键词
stars : individual : LP 944-20; stars; low-mass; brown dwarfs;
D O I
10.1046/j.1365-8711.1998.01642.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Observations are presented which show that Li lambda 6708 is detected with an equivalent width of 0.53 +/- 0.05 Angstrom in the proper-motion object LP 944-20 (which is also known as BRI0337-3535). Hoc is detected in emission at an equivalent width of 1.2 +/- 0.5 Angstrom. The detection of Li implies a mass less than 0.065 M., making this object a brown dwarf. Moreover, the relative weakness of this Li detection (compared to the equivalent widths of 1-2 Angstrom seen in objects of similar spectral type in the Pleiades) implies that Li has been somewhat depleted. This, together with the precisely determined luminosity of LP944-20, implies a mass between 0.056 and 0.064 M., and age between 475 and 650 Myr. This makes it the first brown dwarf to have a well-constrained mass and age determined.
引用
收藏
页码:L42 / L44
页数:3
相关论文
共 28 条