First evidence for a spatially resolved disk structure around the Herbig Ae star R CrA

被引:1
|
作者
Correia, S. [1 ]
Koehler, R. [2 ]
Meeus, G. [1 ]
Zinnecker, H. [1 ]
机构
[1] Astrophys Inst Potsdam, Sternwarte 16, D-14482 Potsdam, Germany
[2] Sterrewacht Leiden, Leiden NL-2333, Netherlands
关键词
D O I
10.1007/978-3-540-74256-2_19
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present mid-infrared interferometric observations of the Herbig Ae star R CrA obtained with MIDI at the VLTI using several projected baselines in the UT2-UT3 configuration. The observations show resolved circurnstellar emission in the wavelength range 8-13 mu m on a similar to 6 AU scale with a non-symmetric intensity distribution, providing support for an inclined disk geometry. Visibilities are best fitted using a uniform ring model with outer radius in the range 6-10 AU, in the wavelength range 8-13 micron. The inclination of the ring with respect to the plane of the sky is found to be similar to 45 degrees, consistent with the 40 degrees suggested from near-infrared imaging polarimetry (Clark et al. 2000, MNRAS, 319, 337).
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页码:175 / 179
页数:5
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