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首页> 外文期刊>The Astrophysical journal >DISCOVERY OF FOUR HIGH PROPER MOTION L DWARFS, INCLUDING A 10?pc L DWARF AT THE L/T TRANSITION* , **
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DISCOVERY OF FOUR HIGH PROPER MOTION L DWARFS, INCLUDING A 10?pc L DWARF AT THE L/T TRANSITION* , **

机译:发现了四个高性能L短波,包括在L / T转换时的10微升L短波*,**

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We discover four high proper motion L dwarfs by comparing the Wide-field Infrared Survey Explorer (WISE) to the Two Micron All Sky Survey. WISE J140533.32+835030.5 is an L dwarf at the L/T transition with a proper motion of 0.85 ± 002?yr–1, previously overlooked due to its proximity to a bright star (V ≈ 12 mag). From optical spectroscopy we find a spectral type of L8, and from moderate-resolution J band spectroscopy we find a near-infrared spectral type of L9. We find WISE J140533.32+835030.5 to have a distance of 9.7 ± 1.7?pc, bringing the number of L dwarfs at the L/T transition within 10?pc from six to seven. WISE J040137.21+284951.7, WISE J040418.01+412735.6, and WISE J062442.37+662625.6 are all early L dwarfs within 25?pc, and were classified using optical and low-resolution near-infrared spectra. WISE J040418.01+412735.6 is an L2 pec (red) dwarf, a member of the class of unusually red L dwarfs. We use follow-up optical and low-resolution near-infrared spectroscopy to classify a previously discovered fifth object WISEP J060738.65+242953.4 as an (L8 Opt/L9 NIR), confirming it as an L dwarf at the L/T transition within 10?pc. WISEP J060738.65+242953.4 shows tentative CH4 in the H band, possibly the result of unresolved binarity with an early T dwarf, a scenario not supported by binary spectral template fitting. If WISEP J060738.65+242953.4 is a single object, it represents the earliest onset of CH4 in the H band of an L/T transition dwarf in the SpeX Library. As very late L dwarfs within 10?pc, WISE J140533.32+835030.5 and WISEP J060738.65+242953.4 will play a vital role in resolving outstanding issues at the L/T transition.
机译:通过将宽视场红外测量仪(WISE)与两微米全天候测量仪进行比较,我们发现了四个高运动L矮星。 WISE J140533.32 + 835030.5是L / T过渡处的L矮星,其适当运动为0.85±002?yr–1,由于它靠近明亮的恒星(V≈12 mag),以前被忽略了。从光谱学中我们可以找到L8的光谱类型,从中等分辨率的J带光谱学中我们可以找到L9的近红外光谱类型。我们发现WISE J140533.32 + 835030.5的距离为9.7±1.7?pc,使L / T过渡处的L矮数从6个变到7个在10μpc内。 WISE J040137.21 + 284951.7,WISE J040418.01 + 412735.6和WISE J062442.37 + 662625.6都是25微秒以内的早期L矮星,并使用光学和低分辨率近红外光谱进行了分类。 WISE J040418.01 + 412735.6是L2 pec(红色)矮人,是异常红色L矮人类别的成员。我们使用后续的光学和低分辨率近红外光谱技术将先前发现的第五个物体WISEP J060738.65 + 242953.4归类为(L8 Opt / L9 NIR),从而确认其为在10片WISEP J060738.65 + 242953.4显示了H波段的暂定CH4,可能是由于早期T矮导致的未解决的二值性,二进制光谱模板拟合不支持这种情况。如果WISEP J060738.65 + 242953.4是单个对象,则它表示SpeX库中L / T过渡矮体H波段中CH4的最早出现。由于L矮度在10?pc以内,因此WISE J140533.32 + 835030.5和WISEP J060738.65 + 242953.4将在解决L / T过渡中的突出问题方面发挥至关重要的作用。

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