Direct Imaging of the Pre-outburst FU Ori Candidate V1331 Cyg

Details Direct Imaging of the Pre-outburst FU Ori Candidate V1331 Cyg Direct Imaging of the Pre-outburst FU Ori Candidate V1331 Cyg

Aug 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1158..135k&link_type=abstract

EXOPLANETS AND DISKS: THEIR FORMATION AND DIVERSITY: Proceedings of the International Conference. AIP Conference Proceedings, V

Physics

Accretion And Accretion Disks, Circumstellar Shells, Clouds, And Expanding Envelopes, Circumstellar Masers, X- And Gamma-Ray Telescopes And Instrumentation, Distances, Redshifts, Radial Velocities, Spatial Distribution Of Galaxies

Scientific paper

We carried out a direct imaging campaign of the pre-outburst FU Ori candidate V1331 Cyg in the H band with CIAO on the Subaru Telescope to investigate the inner structures of VI331 Cyg and to directly detect the disk. Spatial structures revealed by direct imaging may describe the physical conditions of the disk and can restrict the theories of planetary formation. In our preliminary results, we clearly detected a bright arc interior to the known inner ring, which is likely to be the scattered light from the disk. Here, we will show the results and discuss nature of the structure including the comparison with the HST images.

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