CIRCUMBINARY RING, CIRCUMSTELLAR DISKS, AND ACCRETION IN THE BINARY SYSTEM UY AURIGAE

Recent exo-planetary surveys reveal that planets can orbit and survive around binary stars. This suggests that some fraction of young binary systems which possess massive circumbinary (CB) disks may be in the midst of planet formation. However, there are very few CB disks detected. The streaming gas...

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Veröffentlicht in:The Astrophysical journal 2014-09, Vol.793 (1), p.1-14
Hauptverfasser: Tang, Ya-Wen, Dutrey, Anne, Guilloteau, Stephane, PIETU, VINCENT, Di Folco, Emmanuel, Beck, Tracy, Ho, Paul T P, Boehler, Yann, GUETH, FREDERIC, Bary, Jeff, Simon, Michal
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container_end_page 14
container_issue 1
container_start_page 1
container_title The Astrophysical journal
container_volume 793
creator Tang, Ya-Wen
Dutrey, Anne
Guilloteau, Stephane
PIETU, VINCENT
Di Folco, Emmanuel
Beck, Tracy
Ho, Paul T P
Boehler, Yann
GUETH, FREDERIC
Bary, Jeff
Simon, Michal
description Recent exo-planetary surveys reveal that planets can orbit and survive around binary stars. This suggests that some fraction of young binary systems which possess massive circumbinary (CB) disks may be in the midst of planet formation. However, there are very few CB disks detected. The streaming gas accreting from the CB ring toward the CS disks and possible outflows are also identified and resolved. The SO emission is found to be at the bases of the streaming shocks. Our results suggest that the UY Aur system is undergoing an active accretion phase from the CB disk to the CS disks. The UY Aur B might also be a binary system, making the UY Aur a triple system.
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subjects Accretion
Accretion disks
Astrophysics
ASTROPHYSICS, COSMOLOGY AND ASTRONOMY
BINARY STARS
Binary systems
DUSTS
EMISSION
Extrasolar planets
INTERACTIONS
MIXING
ORBITS
Outflow
Physics
PLANETS
PROBES
PROTOPLANETS
RINGS
ROTATION
Sciences of the Universe
Solar and Stellar Astrophysics
WAVELENGTHS
title CIRCUMBINARY RING, CIRCUMSTELLAR DISKS, AND ACCRETION IN THE BINARY SYSTEM UY AURIGAE
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