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An APEX search for carbon emission from NGC 1977 proplyds

Haworth, Thomas J; Kim, Jinyoung S; Qiao, Lin; Winter, Andrew J; Williams, Jonathan P; Clarke, Cathie J; Owen, James E; ... Ballabio, Giulia; + view all (2022) An APEX search for carbon emission from NGC 1977 proplyds. Monthly Notices of the Royal Astronomical Society 10.1093/mnras/stac656. (In press). Green open access

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Abstract

We used the Atacama Pathfinder Experiment (APEX) telescope to search for C I 1-0 (492.16 GHz) emission towards 8 proplyds in NGC 1977, which is an FUV radiation environment two orders of magnitude weaker than that irradiating the Orion Nebular Cluster (ONC) proplyds. C I is expected to enable us to probe the wind launching region of externally photoevaporating discs. Of the 8 targets observed, no 3σ detections of the C I line were made despite reaching sensitivities deeper than the anticipated requirement for detection from prior APEX CI observations of nearby discs and models of external photoevaporation of quite massive discs. By comparing both the proplyd mass loss rates and C I flux constraints with a large grid of external photoevaporation simulations, we determine that the non-detections are in fact fully consistent with the models if the proplyd discs are very low mass. Deeper observations in C I and probes of the disc mass with other tracers (e.g. in the continuum and CO) can test this. If such a test finds higher masses, this would imply carbon depletion in the outer disc, as has been proposed for other discs with surprisingly low C I fluxes, though more massive discs would also be incompatible with models that can explain the observed mass loss rates and C I non-detections. The expected remaining lifetimes of the proplyds are estimated to be similar to those of proplyds in the ONC at 0.1 Myr. Rapid destruction of discs is therefore also a feature of common, intermediate UV environments.

Type: Article
Title: An APEX search for carbon emission from NGC 1977 proplyds
Open access status: An open access version is available from UCL Discovery
DOI: 10.1093/mnras/stac656
Publisher version: https://doi.org/10.1093/mnras/stac656
Language: English
Additional information: This version is the author accepted manuscript. For information on re-use, please refer to the publisher's terms and conditions.
UCL classification: UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Physics and Astronomy
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL
URI: https://discovery.ucl.ac.uk/id/eprint/10145384
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