研究成果藝廊 > 恆星形成

研究成果藝廊

恆星形成

總覽
更新 [須登入]

Dust distribution in the binary protostellar system L1551 NE observed with the SMA in 0.9 mm continuum.

圖片來源: Shigehisa Takakuwa

Dust distribution in the binary protostellar system L1551 NE observed with the SMA in 0.9 mm continuum. Crosses show the position of each binary component. Dashed curves delineate the ring-like “circumbinary disk” components. (Takakuwa et al. 2012, ApJ, 754, 52)