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Connecting the dots: a correlation between ionizing radiation and cloud mass-loss rate traced by optical integral field spectroscopy

McLeod, A.F.; Gritschneder, M.; Dale, J.E.; Ginsburg, A.; Klaassen, P.D.; Mottram, J.C.; Preibisch, T.; Ramsay, S.; Reiter, M.; Testi, L.

Authors

M. Gritschneder

J.E. Dale

A. Ginsburg

P.D. Klaassen

J.C. Mottram

T. Preibisch

S. Ramsay

M. Reiter

L. Testi



Abstract

We present an analysis of the effect of feedback from O- and B-type stars with data from the integral field spectrograph Multi Unit Spectroscopic Explorer (MUSE) mounted on the Very Large Telescope of pillar-like structures in the Carina Nebular Complex, one of the most massive star-forming regions in the Galaxy. For the observed pillars, we compute gas electron densities and temperatures maps, produce integrated line and velocity maps of the ionized gas, study the ionization fronts at the pillar tips, analyse the properties of the single regions, and detect two ionized jets originating from two distinct pillar tips. For each pillar tip, we determine the incident ionizing photon flux Q0, pil originating from the nearby massive O- and B-type stars and compute the mass-loss rate M˙ of the pillar tips due to photoevaporation caused by the incident ionizing radiation. We combine the results of the Carina data set with archival MUSE data of a pillar in NGC 3603 and with previously published MUSE data of the Pillars of Creation in M16, and with a total of 10 analysed pillars, find tight correlations between the ionizing photon flux and the electron density, the electron density and the distance from the ionizing sources, and the ionizing photon flux and the mass-loss rate. The combined MUSE data sets of pillars in regions with different physical conditions and stellar content therefore yield an empirical quantification of the feedback effects of ionizing radiation. In agreement with models, we find that M˙∝Q1/20,pil
⁠.

Citation

McLeod, A., Gritschneder, M., Dale, J., Ginsburg, A., Klaassen, P., Mottram, J., …Testi, L. (2016). Connecting the dots: a correlation between ionizing radiation and cloud mass-loss rate traced by optical integral field spectroscopy. Monthly Notices of the Royal Astronomical Society, 462(4), https://doi.org/10.1093/mnras/stw1864

Journal Article Type Article
Online Publication Date Jul 30, 2016
Publication Date 2016
Deposit Date Oct 24, 2022
Journal Monthly Notices of the Royal Astronomical Society
Print ISSN 0035-8711
Electronic ISSN 1365-2966
Publisher Royal Astronomical Society
Volume 462
Issue 4
DOI https://doi.org/10.1093/mnras/stw1864
Public URL https://durham-repository.worktribe.com/output/1190885