The structure of pre-transitional protoplanetary disks. II. Azimuthal asymmetries, different radial distributions of large and small dust grains in pds 70

J. Hashimoto, T. Tsukagoshi, J. M. Brown, R. Dong, T. Muto, Z. Zhu, J. Wisniewski, N. Ohashi, T. Kudo, N. Kusakabe, L. Abe, E. Akiyama, W. Brandner, T. Brandt, J. Carson, T. Currie, S. Egner, M. Feldt, C. A. Grady, O. GuyonY. Hayano, M. Hayashi, S. Hayashi, T. Henning, K. Hodapp, M. Ishii, M. Iye, M. Janson, R. Kandori, G. Knapp, M. Kuzuhara, J. Kwon, T. Matsuo, M. W. McElwain, S. Mayama, K. Mede, S. Miyama, J. I. Morino, A. Moro-Martin, T. Nishimura, T. S. Pyo, G. Serabyn, T. Suenaga, H. Suto, R. Suzuki, Y. Takahashi, M. Takami, N. Takato, H. Terada, C. Thalmann, D. Tomono, E. L. Turner, M. Watanabe, T. Yamada, H. Takami, T. Usuda, M. Tamura

Research output: Contribution to journalArticle

27 Scopus citations

Abstract

The formation scenario of a gapped disk, i.e., transitional disk, and its asymmetry is still under debate. Proposed scenarios such as disk-planet interaction, photoevaporation, grain growth, anticyclonic vortex, eccentricity, and their combinations would result in different radial distributions of the gas and the small (sub-μm size) and large (millimeter size) dust grains as well as asymmetric structures in a disk. Optical/near-infrared (NIR) imaging observations and (sub-)millimeter interferometry can trace small and large dust grains, respectively; therefore multi-wavelength observations could help elucidate the origin of complicated structures of a disk. Here we report Submillimeter Array observations of the dust continuum at 1.3 mm and 12CO J = 2 → 1 line emission of the pre-transitional protoplanetary disk around the solar-mass star PDS 70. PDS 70, a weak-lined T Tauri star, exhibits a gap in the scattered light from its disk with a radius of ∼65 AU at NIR wavelengths. However, we found a larger gap in the disk with a radius of ∼80 AU at 1.3 mm. Emission from all three disk components (the gas and the small and large dust grains) in images exhibits a deficit in brightness in the central region of the disk, in particular, the dust disk in small and large dust grains has asymmetric brightness. The contrast ratio of the flux density in the dust continuum between the peak position to the opposite side of the disk reaches 1.4. We suggest the asymmetries and different gap radii of the disk around PDS 70 are potentially formed by several (unseen) accreting planets inducing dust filtration.

Original languageEnglish (US)
Article number43
JournalAstrophysical Journal
Volume799
Issue number1
DOIs
StatePublished - Jan 20 2015
Externally publishedYes

Keywords

  • planetary systems
  • polarization
  • protoplanetary disks
  • stars: individual (PDS 70)
  • stars: pre-main sequence
  • submillimeter: general

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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    Hashimoto, J., Tsukagoshi, T., Brown, J. M., Dong, R., Muto, T., Zhu, Z., Wisniewski, J., Ohashi, N., Kudo, T., Kusakabe, N., Abe, L., Akiyama, E., Brandner, W., Brandt, T., Carson, J., Currie, T., Egner, S., Feldt, M., Grady, C. A., ... Tamura, M. (2015). The structure of pre-transitional protoplanetary disks. II. Azimuthal asymmetries, different radial distributions of large and small dust grains in pds 70. Astrophysical Journal, 799(1), [43]. https://doi.org/10.1088/0004-637X/799/1/43