The Astrophysical Journal Letters (Jan 2023)

ALMA Survey of Orion Planck Galactic Cold Clumps (ALMASOP): A Forming Quadruple System with Continuum “Ribbons” and Intricate Outflows

  • Qiu-yi Luo,
  • Tie Liu,
  • Aaron T. Lee,
  • Stella S. R. Offner,
  • James di Francesco,
  • Doug Johnstone,
  • Mika Juvela,
  • Paul F. Goldsmith,
  • Sheng-Li Qin,
  • Xiaofeng Mai,
  • Xun-chuan Liu,
  • Patricio Sanhueza,
  • Feng-Wei Xu,
  • Ken’ichi Tatematsu,
  • Somnath Dutta,
  • Huei-Ru Vivien Chen,
  • Shanghuo Li,
  • Aiyuan Yang,
  • Sheng-Yuan Liu,
  • Chin-Fei Lee,
  • Naomi Hirano,
  • Chang Won Lee,
  • Dipen Sahu,
  • Hsien Shang,
  • Shih-Ying Hsu,
  • Leonardo Bronfman,
  • Woojin Kwon,
  • M. G. Rawlings,
  • David Eden,
  • Xing Lu,
  • Qi-lao Gu,
  • Zhiyuan Ren,
  • D. Ward-Thompson,
  • Zhi-Qiang Shen

DOI
https://doi.org/10.3847/2041-8213/acdddf
Journal volume & issue
Vol. 952, no. 1
p. L2

Abstract

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One of the most poorly understood aspects of low-mass star formation is how multiple-star systems are formed. Here we present the results of Atacama Large Millimeter/submillimeter Array (ALMA) Band 6 observations toward a forming quadruple protostellar system, G206.93-16.61E2, in the Orion B molecular cloud. ALMA 1.3 mm continuum emission reveals four compact objects, of which two are Class I young stellar objects and the other two are likely in prestellar phase. The 1.3 mm continuum emission also shows three asymmetric ribbon-like structures that are connected to the four objects, with lengths ranging from ∼500 to ∼2200 au. By comparing our data with magnetohydrodynamic simulations, we suggest that these ribbons trace accretion flows and also function as gas bridges connecting the member protostars. Additionally, ALMA CO J = 2−1 line emission reveals a complicated molecular outflow associated with G206.93-16.61E2, with arc-like structures suggestive of an outflow cavity viewed pole-on.

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