| タイトル | Polarimetric Imaging of Large Cavity Structures in the Pre-transitional Protoplanetary Disk around PDS 70: Observations of the Disk |
| 本文（外部サイト） | http://hdl.handle.net/2060/20120016564 |
| 著者（英） | Dong, R.; Kusakabe,N.; Knapp G.; Iye, M.; Suto, H.; Hayashi, M.; Suzuki, R.; Serabyn, G.; McElwain, M. W.; Janson, M.; Hashimoto, J.; Morino, J.-I.; Tamura, M.; Turner, E. L.; Kandori, R.; Brandt, T.; Zhu, Z. |
| 著者所属（英） | NASA Goddard Space Flight Center |
| 発行日 | 2012-01-01 |
| 言語 | eng |
| 内容記述 | We present high resolution H-band polarized intensity (PI; FWHM = 0."1: 14 AU) and L'-band imaging data (FWHM = 0."11: 15 AU) of the circumstellar disk around the weak-lined T Tauri star PDS 70 in Centaurus at a radial distance of 28 AU (0."2) up to 210 AU (1."5). In both images, a giant inner gap is clearly resolvro for the first time, and the radius of the gap is approx 70 AU. Our data show that the geometric center of the disk shifts by approx 6 AU toward the minor axis. We confirm that the brown dwarf companion candidate to the north of PDS 70 is a background star based on its proper motion. As a result of SED fitting by Monte Carlo radiative transfer modeling, we infer the existence of an optically thick inner disk at a few AU. Combining our observations and modeling, we classify the disk of PDS 70 as a pre-transitional disk. Furthermore, based on the analysis of L'-band imaging data, we put an upper limit mass of companions at approx 30 to approx 50M(sub J) within the gap. Taking account of the presence of the large and sharp gap, we suggest that the gap could be formed by dynamical interactions of sub-stellar companions or multiple unseen giant planets in the gap. |
| NASA分類 | Astronomy |
| レポートNO | GSFC.JA.7392.2012 |
| 権利 | Copyright, Distribution under U.S. Government purpose rights |
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