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Illuminating evaporating protostellar outflows: ERIS/SPIFFIER reveals the dissociation and ionization of HH 900

Reiter, Megan; Haworth, Thomas J; Manara, Carlo F; Ramsay, Suzanne; Klaassen, Pamela D; Itrich, Dominika; McLeod, Anna F

Illuminating evaporating protostellar outflows: ERIS/SPIFFIER reveals the dissociation and ionization of HH 900 Thumbnail


Authors

Megan Reiter

Thomas J Haworth

Carlo F Manara

Suzanne Ramsay

Pamela D Klaassen

Dominika Itrich



Abstract

Protostellar jets and outflows are signposts of active star formation. In H II regions, molecular tracers like CO only reveal embedded portions of the outflow. Outside the natal cloud, outflows are dissociated, ionized, and eventually completely ablated, leaving behind only the high-density jet core. Before this process is complete, there should be a phase where the outflow is partially molecular and partially ionized. In this paper, we capture the HH 900 outflow while this process is in action. New observations from the Enhanced Resolution Imager and Spectrograph/SPIFFIER near-infrared (IR) integral field unit spectrograph using the K-middle filter (λ = 2.06–2.34 μm) reveal H2 emission from the dissociating outflow and Br-γ tracing its ionized skin. Both lines trace the wide-angle outflow morphology but H2 only extends ∼5000 au into the H II region while Br-γ extends the full length of the outflow (∼12 650 au), indicating rapid dissociation of the molecules. H2 has higher velocities further from the driving source, consistent with a jet-driven outflow. Diagnostic line ratios indicate that photoexcitation, not just shocks, contributes to the excitation in the outflow. We argue that HH 900 is the first clear example of an evaporating molecular outflow and predict that a large column of neutral material that may be detectable with Atacama Large Millimeter Array accompanies the dissociating molecules. Results from this study will help guide the interpretation of near-IR images of externally irradiated jets and outflows such as those obtained with the JWST in high-mass star-forming regions where these conditions may be common.

Citation

Reiter, M., Haworth, T. J., Manara, C. F., Ramsay, S., Klaassen, P. D., Itrich, D., & McLeod, A. F. (2024). Illuminating evaporating protostellar outflows: ERIS/SPIFFIER reveals the dissociation and ionization of HH 900. Monthly Notices of the Royal Astronomical Society, 527(2), 3220–3230. https://doi.org/10.1093/mnras/stad3304

Journal Article Type Article
Acceptance Date Oct 24, 2023
Online Publication Date Oct 28, 2023
Publication Date 2024-01
Deposit Date Jan 31, 2024
Publicly Available Date Jan 31, 2024
Journal Monthly Notices of the Royal Astronomical Society
Print ISSN 0035-8711
Electronic ISSN 1365-2966
Publisher Royal Astronomical Society
Peer Reviewed Peer Reviewed
Volume 527
Issue 2
Pages 3220–3230
DOI https://doi.org/10.1093/mnras/stad3304
Public URL https://durham-repository.worktribe.com/output/2188313
Publisher URL https://doi.org/10.1093/mnras/stad3304

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Copyright Statement
© 2023 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society. This is an Open Access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium,
provided the original work is properly cited.





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