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Article Dans Une Revue The Astrophysical Journal Année : 2020

High-resolution Near-infrared Polarimetry and Submillimeter Imaging of FS Tau A: Possible Streamers in Misaligned Circumbinary Disk System

Frantz Martinache
Yi Yang
Eiji Akiyama
Jun Hashimoto
Saeko Hayashi
  • Fonction : Auteur
Carol Grady
Markus Janson
Nemanja Jovanovic
Taichi Uyama
Takao Nakagawa
Nobuhiko Kusakabe
  • Fonction : Auteur
Timothy Brandt
Michael Bonnefoy
  • Fonction : Auteur
Joseph Carson
  • Fonction : Auteur
Evan Rich
Markus Feldt
  • Fonction : Auteur
Miwa Goto
  • Fonction : Auteur
Tyler Groff
Olivier Guyon
Yutaka Hayano
Masahiko Hayashi
  • Fonction : Auteur
Thomas Henning
Klaus Hodapp
Miki Ishii
  • Fonction : Auteur
Masanori Iye
Ryo Kandori
Jeremy Kasdin
Gillian Knapp
Jungmi Kwon
Julien Lozi
Taro Matsuo
  • Fonction : Auteur
Satoshi Mayama
Michael Mcelwain
Shoken Miyama
Jun-Ichi Morino
  • Fonction : Auteur
Amaya Moro-Martin
Tetsuo Nishimura
  • Fonction : Auteur
Tae-Soo Pyo
Eugene Serabyn
  • Fonction : Auteur
Hiroshi Suto
  • Fonction : Auteur
Ryuji Suzuki
  • Fonction : Auteur
Michihiro Takami
Naruhisa Takato
  • Fonction : Auteur
Hiroshi Terada
Christian Thalmann
Edwin Turner
  • Fonction : Auteur
Makoto Watanabe
John Wisniewski
Toru Yamada
  • Fonction : Auteur
Hideki Takami
  • Fonction : Auteur
Tomonori Usuda
Motohide Tamura

Résumé

Abstract We analyzed the young (2.8 Myr-old) binary system FS Tau A using near-infrared ( H -band) high-contrast polarimetry data from Subaru/HiCIAO and submillimeter CO (J = 2–1) line emission data from Atacama Large Millimeter/submillimeter Array (ALMA). Both the near-infrared and submillimeter observations reveal several clear structures extending to ∼240 au from the stars. Based on these observations at different wavelengths, we report the following discoveries. One arm-like structure detected in the near-infrared band initially extends from the south of the binary with a subsequent turn to the northeast, corresponding to two bar-like structures detected in ALMA observations with an local standard of rest kinematic (LSRK) velocity of 1.19–5.64 km s −1 . Another feature detected in the near-infrared band extends initially from the north of the binary, relating to an arm-like structure detected in ALMA observations with an LSRK velocity of 8.17–16.43 km s −1 . From their shapes and velocities, we suggest that these structures can mostly be explained by two streamers that connect the outer circumbinary disk and the central binary components. These discoveries will be helpful for understanding the evolution of streamers and circumstellar disks in young binary systems.
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hal-03518334 , version 1 (12-01-2022)

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Frantz Martinache, Yi Yang, Eiji Akiyama, Thayne Currie, Ruobing Dong, et al.. High-resolution Near-infrared Polarimetry and Submillimeter Imaging of FS Tau A: Possible Streamers in Misaligned Circumbinary Disk System. The Astrophysical Journal, 2020, 889 (2), pp.140. ⟨10.3847/1538-4357/ab64f9⟩. ⟨hal-03518334⟩
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