Issue |
A&A
Volume 688, August 2024
|
|
---|---|---|
Article Number | A201 | |
Number of page(s) | 16 | |
Section | Interstellar and circumstellar matter | |
DOI | https://doi.org/10.1051/0004-6361/202451011 | |
Published online | 23 August 2024 |
Investigation of the rotational spectrum of CH3 17OH and its tentative detection toward Sagittarius B2(N)*
1
Astrophysik/I. Physikalisches Institut, Universität zu Köln,
Zülpicher Str. 77,
50937
Köln,
Germany
e-mail: hspm@ph1.uni-koeln.de
2
Institute of Radio Astronomy of NASU,
Mystetstv 4,
61002
Kharkiv,
Ukraine
e-mail: ilyushin@rian.kharkov.ua
3
Max-Planck-Institut für Radioastronomie,
Auf dem Hügel 69,
53121
Bonn,
Germany
Received:
6
June
2024
Accepted:
28
June
2024
Context. Methanol is an abundant and widespread molecule in the interstellar medium. The column density of its 18O isotopolog, CH318OH, is in some star-forming regions so high that the search for CH317OH is promising. But only very few transition frequencies of CH317 OH with a microwave accuracy have been published prior to our investigation.
Aims. We want to extend the very limited rotational line list of CH317OH to be able to search for this isotopolog in the interstellar medium.
Methods. We recorded the rotational spectrum of CH317OH between 38 and 1095 GHz employing a methanol sample enriched in 17O to 20%. A torsion-rotation Hamiltonian model based on the rho-axis method was employed to fit the data, as in our previous studies. We searched for rotational transitions of CH317OH in the imaging spectral line survey ReMoCA obtained with the Atacama Large Millimeter/submillimeter Array (ALMA) toward the high-mass star-forming region Sgr B2(N). The observed spectra were modeled under the assumption of local thermodynamic equilibrium (LTE).
Results. The assignments cover 0 ≤ J ≤ 45, Ka ≤ 16, and mainly the vt = 0 and 1 torsional states. The Hamiltonian model describes our data well. The model was applied to derive a line list for radio-astronomical observations. We report a tentative detection of CH317OH along with secure detections of the more abundant isotopologs of methanol toward Sgr B2(N2b). The derived column densities yield isotopic ratios 12C/13C = 25, 16O/18O = 240, and 18O/17O = 3.3, which are consistent with values found earlier for other molecules in Sgr B2.
Conclusions. The agreement between the 18O/17O isotopic ratio that we obtained for methanol and the 18O/17O ratios reported in the past for other molecules in Sgr B2(N) strongly supports our tentative interstellar identification of CH317OH. The accuracy of the derived line list is sufficient for further radio astronomical searches for this methanol isotopolog toward other star-forming regions.
Key words: astrochemistry / molecular data / methods: laboratory: molecular / techniques: spectroscopic / ISM: molecules / radio lines: ISM
Electronic supplementary material for this work can be found at https://doi.org/10.5281/zenodo.12581728
© The Authors 2024
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.
This article is published in open access under the Subscribe to Open model. Subscribe to A&A to support open access publication.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.