학술논문
ALMA Survey of Orion Planck Galactic Cold Clumps (ALMASOP): A forming quadruple system with continuum `ribbons' and intricate outflows
Document Type
Working Paper
Author
Luo, Qiu-yi; Liu, Tie; Lee, Aaron T.; Offner, Stella S. R.; di Francesco, James; Johnstone, Doug; Juvela, Mika; Goldsmith, Paul F.; Qin, Sheng-Li; Mai, Xiaofeng; Liu, Xun-chuan; Sanhueza, Patricio; Xu, Feng-Wei; Tatematsu, Ken'ichi; Dutta, Somnath; Chen, Huei-Ru Vivien; Li, Shanghuo; Yang, Aiyuan; Liu, Sheng-Yuan; Lee, Chin-Fei; Hirano, Naomi; Lee, Chang Won; Sahu, Dipen; Shang, Hsien; Hsu, Shih-Ying; Bronfman, Leonardo; Kwon, Woojin; Rawlings, M. G.; Eden, David; Lu, Xing; Gu, Qi-lao; Ren, Zhiyuan; Ward-Thompson, D; Shen, Zhi-Qiang
Source
Subject
Language
Abstract
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 towards 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 (YSOs), 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 $\sim$500 au to $\sim$2200 au. By comparing our data with magneto-hydrodynamic (MHD) 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.
Comment: The paper was accepted by APJL
Comment: The paper was accepted by APJL