Image Details
Caption: Figure 5.
Filaments (green lines) overlaid on 850 μm continuum toward (a) 2264C and (b) 2264D. The cyan contours mark 0.1, 0.2, 0.5, 1.0, 2.0, 5.0, and 10 mJy arcsec−2. The red and yellow stars label IRS1 (zero-age main-sequence) and IRS2 (class I), the dominating sources in 2264C and 2264D, respectively. We note that IRS2 is offset from any filament or intensity peak, while IRS1 is at the converging point of multiple filaments. The main filaments along the prevailing directions are labeled.
© 2024. The Author(s). Published by the American Astronomical Society.