Purser, SJD, Lumsden, SL orcid.org/0000-0001-5748-5166, Hoare, MG orcid.org/0000-0003-2684-399X et al. (1 more author) (2021) A Galactic survey of radio jets from massive protostars. Monthly Notices of the Royal Astronomical Society, 504 (1). pp. 338-355. ISSN 0035-8711
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 (∼0.04 arcsec) Jansky Very Large Array observations towards two subsamples of massive star-forming regions of different evolutionary statuses: 48 infrared-bright, massive, young, stellar objects (MYSOs) and 8 infrared dark clouds (IRDCs) containing 16 luminous (Lbol>103L⊙) cores. For 94 per cent of the MYSO sample, we detect thermal radio (α ≥ −0.1 whereby Sν ∝ να) sources coincident with the protostar, of which 84 per cent (13 jets and 25 candidates) are jet like. Radio luminosity is found to scale with Lbol similarly to the low-mass case supporting a common mechanism for jet production across all masses. Associated radio lobes tracing shocks are seen towards 52 per cent 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 m˙jet∝Lbol0.9±0.2, 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 pjet > poutflow. Finally, from their physical extent we show that the radio emission cannot originate from small, optically thick H II regions. Towards the IRDC cores, we observe increasing incidence rates/radio fluxes with age using the proxy of increasing luminosity-to-mass (L/M) and decreasing infrared flux ratios (S70μm/S24μm). Cores with (L/M)<40L⊙M⊙−1 are not detected above (5.8GHz) radio luminosities of ∼1mJykpc2.
Metadata
Item Type: | Article |
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Authors/Creators: |
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Copyright, Publisher and Additional Information: | © 2021 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society. This is an author produced version of an article published in Monthly Notices of the Royal Astronomical Society. Uploaded in accordance with the publisher's self-archiving policy. |
Keywords: | surveys; stars: formation; stars: massive; stars: protostars; ISM: jets and outflows; radio continuum: ISM |
Dates: |
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Institution: | The University of Leeds |
Academic Units: | The University of Leeds > Faculty of Engineering & Physical Sciences (Leeds) > School of Physics and Astronomy (Leeds) > Astrophysics (Leeds) |
Funding Information: | Funder Grant number STFC (Science and Technology Facilities Council) ST/I001557/1 STFC (Science and Technology Facilities Council) ST/L000628/1 STFC (Science and Technology Facilities Council) ST/P00041X/1 STFC (Science and Technology Facilities Council) Not Known |
Depositing User: | Symplectic Publications |
Date Deposited: | 27 May 2021 12:01 |
Last Modified: | 25 Jun 2023 22:40 |
Status: | Published |
Publisher: | Oxford University Press (OUP) |
Identification Number: | 10.1093/mnras/stab747 |
Open Archives Initiative ID (OAI ID): | oai:eprints.whiterose.ac.uk:174495 |