A Galactic survey of radio jets from massive protostars
arXiv:2103.08990 · doi:10.1093/mnras/stab747
Abstract
In conjunction with a previous southern-hemisphere work, we present the largest radio survey of jets from massive protostars to date with high-resolution, () VLA observations towards two subsamples of massive star-forming regions of different evolutionary statuses: 48 infrared-bright, massive YSOs and 8 IRDCs containing 16 luminous () cores. For of the MYSO sample we detect thermal radio ( whereby ) sources coincident with the protostar, of which (13 jets and 25 candidates) are jet-like. Radio luminosity is found to scale with similarly to the low-mass case supporting a common mechanism for jet production across all masses. Associated radio lobes tracing shocks are seen towards of jet-like objects and are preferentially detected towards jets of higher radio and bolometric luminosities, resulting from our sensitivity limitations. We find jet mass loss rate scales with bolometric luminosity as , thereby discarding radiative, line-driving mechanisms as the dominant jet-launching process. Calculated momenta show that the majority of jets are mechanically capable of driving the massive, molecular outflow phenomena since . Finally, from their physical extent we show that the radio emission can not originate from small, optically-thick \textsc{Hii} regions. Towards the IRDC cores, we observe increasing incidence rates/radio fluxes with age using the proxy of increasing luminosity-to-mass and decreasing infrared flux ratios . Cores with are not detected above () radio luminosities of .
To be published in MNRAS. 20 pages main text (4 tables, 14 figures), 90 pages appendices (6 tables, 66 figures)
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