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首页> 外文期刊>The Astrophysical journal >A Possible Brown Dwarf Companion to the White Dwarf GD 1400
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A Possible Brown Dwarf Companion to the White Dwarf GD 1400

机译:白矮星GD 1400可能的棕矮星伴侣

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An unresolved, likely L dwarf companion to the DA white dwarf GD 1400 is reported. This would be only the second such system known, discovered 17 years after the prototype L dwarf, GD 165B, was determined to be a companion to a white dwarf. Photometric observations and model-predicted of the well-studied white dwarf primary stellar parameters indicate that GD 1400B has J - K 2.0 and MK = 12.13 mag. If correct, this would place GD 1400B at spectral type L6, and it would be the lowest-luminosity unevolved companion known to a white dwarf and thus a definite brown dwarf. However, a low-resolution Keck NIRSPEC 2.1–2.4 μm spectrum may not be consistent with known L dwarfs. Uncertainties in classification will remain until the binary is resolved or a trigonometric parallax is measured.
机译:据报道,DA白矮星GD 1400有一个尚未解决的,可能是L矮星的伴侣。这只是已知的第二个此类系统,是在原型L矮人GD 165B被确定为白矮星的伴侣之后17年才发现的。研究充分的白矮星主要恒星参数的光度观测和模型预测表明,GD 1400B的J-K 2.0和MK = 12.13 mag。如果正确的话,这会将GD 1400B置于光谱类型L6,这将是白矮星和因此确定的棕矮星已知的最低发光度的未进化同伴。但是,低分辨率的Keck NIRSPEC 2.1–2.4μm光谱可能与已知的L矮星不一致。分类的不确定性将一直存在,直到解析二进制文件或测量三角视差为止。

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