Near-Infrared Imaging Polarimetry of LkCa 15: A Possible Warped Inner Disk
Daehyeon Oh, Jun Hashimoto, Motohide Tamura, John Winsiewski, Eiji, Akiyama, Thayne Currie, Satoshi Mayama, Michihiro Takami, Christian Thalmann,, Tomoyuki Kudo, Nobuhiko Kusakabe, Lyu Abe, Wolfgang Brandner, Timothy D., Brandt, Joseph C. Carson, Sebastian Egner, Markus Feldt

TL;DR
This study uses high-contrast near-infrared imaging to reveal a warped inner disk and a large gap in the transitional disk around LkCa 15, suggesting the presence of multiple planets.
Contribution
First high-resolution polarized imaging showing a warped inner disk and a confirmed large gap in LkCa 15's disk.
Findings
Resolved a gap of <~27 AU at ~48 AU from the star
Confirmed a misaligned, possibly warped, inner disk
Suggests existence of multiple planets with mass <~1 Mjup
Abstract
We present high-contrast H-band polarized intensity images of the transitional disk around the young solar-like star LkCa 15. By utilizing Subaru/HiCIAO for polarimetric differential imaging, both the angular resolution and the inner working angle reach 0.07" and r=0.1", respectively. We obtained a clearly resolved gap (width <~ 27 AU) at ~ 48 AU from the central star. This gap is consistent with images reported in previous studies. We also confirmed the existence of a bright inner disk with a misaligned position angle of 13+/-4 degree with respect to that of the outer disk, i.e., the inner disk is possibly warped. The large gap and the warped inner disk both point to the existence of a multiple planetary system with a mass of <~1Mjup.
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