Issue |
A&A
Volume 669, January 2023
|
|
---|---|---|
Article Number | L7 | |
Number of page(s) | 5 | |
Section | Letters to the Editor | |
DOI | https://doi.org/10.1051/0004-6361/202245358 | |
Published online | 09 January 2023 |
Analysis of the first infrared spectrum of quasi-bound H2 line emission in Herbig-Haro 7
1
Sorbonne Université, Observatoire de Paris, PSL University, CNRS, LERMA, 5 place Janssen, 92190 Meudon Cedex, France
e-mail: evelyne.roueff@obspm.fr
2
Armagh Observatory and Planetarium, College Hill, Armagh BT61 9DB, Northern Ireland
e-mail: Michael.Burton@Armagh.ac.uk
3
Gemini Obsevatory/NSF’s NOIRLab, 670 N. A’ohoku Place, Hilo, HI 96720, USA
e-mail: tom.geballe@noirlab.edu
Received:
2
November
2022
Accepted:
20
December
2022
Context. Highly excited molecular hydrogen (H2) has been observed in many regions of shocked molecular gas. A recently published K-band spectrum of Herbig-Haro 7 (HH7) contains several vibration-rotation lines of H2 from highly excited energy levels that have not been detected elsewhere, including a line at 2.179 μm identified as arising from the v = 2, J = 29 level, which lies above the dissociation limit of H2. One emission line at 2.104 μm in this spectrum was unidentified.
Aims. We aim to complete the analysis of the spectrum of HH7 by including previously missing molecular data that have been recently computed.
Methods. We re-analysed the K-band spectrum, emphasising the physics of quasi-bound upper levels that can produce infrared emission lines in the K band.
Results. We confirm the identification of the 2 − 1 S(27) line at 2.1785 μm and identify the line at 2.1042 μm as due to the 1−0 S(29) transition of H2, whose upper level energy is also higher than the dissociation limit. This latter identification, its column density, and the energy of its upper level further substantiate the existence of a hot thermal component at 5000 K in the HH7 environment.
Conclusions. The presence of the newly identified 1 − 0 S(29) line, whose quasi-bound upper level (v = 1, J = 31) has a significant spontaneous dissociation probability, shows that dissociation of H2 is occurring. The mechanism by which virtually all of the H2 in levels with energies from 20 000 K to 53 000 K is maintained in local thermodynamic equilibrium at a single temperature of ∼5000 K remains to be understood.
Key words: astrochemistry / molecular data / ISM: molecules / ISM: jets and outflows
© The Authors 2023
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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