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首页> 外文期刊>Astronomische Nachrichten: A Journal on all Fields of Astronomy >Anti-solar differential rotation and surface flow pattern on UZ Librae
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Anti-solar differential rotation and surface flow pattern on UZ Librae

机译:UZ Librae的反太阳差速旋转和表面流型

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Were-investigate UZ Libr ae spectra obtained at KPNO in 1998 and 2000. From the 1998 data we compose 11 consecutive Doppler images using the Ca I-6439, Fe I-6393 and Fe I-6411 lines. Applying the method of average cross-correlation of contiguous Doppler images we find anti-solar differential rotation with a surface shear of alpha approximate to -0.03. The pilot application of the local correlation tracking technique for the same data qualitatively confirms this result and indicates complex flow pattern on the stellar surface. From the cross-correlation of the two available Doppler images in 2000 we also get anti-solar differential rotation but with a much weaker shear of alpha approximate to -0.004. (c) 2007 WILEY-VCH Verlag GmbH&Co. KGaA, Weinheim.
机译:我们分别研究了1998和2000年在KPNO获得的UZ Libr ae光谱。根据1998年的数据,我们使用Ca I-6439,Fe I-6393和Fe I-6411谱线组成了11个连续的多普勒图像。应用连续多普勒图像的平均互相关方法,我们发现反太阳微分旋转,其表面剪切α约为-0.03。对于相同的数据,局部相关性跟踪技术的试验应用从质量上证实了这一结果,并指出了恒星表面上的复杂流型。从2000年的两个可用多普勒图像的互相关中,我们还得到了反太阳微分旋转,但alpha的剪切强度弱得多,约为-0.004。 (c)2007 WILEY-VCH Verlag GmbH&Co。魏因海姆(Kain)

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