Free Access

Fig. 12


CARMA continuum observations of NGC 1333/IRAS 4C at 1.3 mm (grayscale) overplotted with the red and blue wings of 13CO 21. The velocity range of the line is between +5 and +11 km s-1, and a siginificant part of the emission has been resolved out by the interferometer at the source velocity, while we still detect emission from the wings. The peaks of the blue (from +5 to +6.5 km s-1) and red (from +8.5 to +11 km s-1) wing show a small offset compared to the peak intensity of the continuum. The blue contours levels are set to 0.04, 0.06, 0.08, 0.10, and 0.13 Jy/beam (rms ~ 0.014 Jy/beam) and the red at 0.06, 0.09, 0.12, 0.15, and 0.18 Jy/beam (rms ~ 0.02 Jy/beam). The ellipse shows the beam size and shape at this wavelength (2.12× 1.81). The arrows represent the direction of blue- and redshifted outflow components (Tobin et al. 2015).

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.