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First Results from ALPPS: A Sub-Alfvénic Streamer in SVS 13A

  • Authors: P. C. Cortés, J. E. Pineda, T.-H. Hsieh, J. J. Tobin, P. Saha, J. M. Girart, V. J. M. Le Gouellec, I. W. Stephens, L. W. Looney, E. Koumpia, M. T. Valdivia-Mena, L. Cacciapuoti, C. Gieser, S. S. R. Offner, P. Caselli, P. Sanhueza, D. Segura-Cox, M. Fernández-López, K. Morii, B. Huang, F. O. Alves, Q. Zhang, W. Kwon, C. L. H. Hull, Z.-Y. Li

P. C. Cortés et al 2025 The Astrophysical Journal Letters 992 .

  • Provider: AAS Journals

Caption: Figure 14.

Left panel: the C18O moment 1 map shown with robust = 0.5 in color scale, where the velocities are relative to vlsr = 7.36 km s−1. Superposed in yellow pseudovectors is the velocity gradient, which was computed over the moment 1 map. Also, superposed in magenta pseudovectors is the inferred magnetic field as derived from the polarized emission, also imaged using robust = 0.5. In contours, we show the total intensity of the continuum emission. Right panel: same as the left panel but with the polarization position angle as black pseudovectors. The beam is depicted as a blue ellipse in the bottom left corner, and the scale is displayed in the bottom right corner of each panel.

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