The Discovery of 25 <i>μ</i>m Interstellar Methanol

Abstract We present the first astrophysical detection of methanol (CH 3 OH) in the torsional band near 25 μ m. Using high-resolution mid-infrared (MIR) spectroscopy, we identified over 70 gas-phase CH 3 OH absorption lines between 20 and 28 μ m toward the massive protostar NGC 7538 IRS 1 with the Stratospheric Observatory for Infrared Astronomy/Echelon-Cross-Echelle Spectrograph. We derive a temperature of 180 K and a total column density of 2 × 10 17 cm −2 , comparable to submillimeter measurements. Complementary analysis of acetylene (C 2 H 2 ) absorption lines is also included. Both CH 3 OH and C 2 H 2 reveal an unresolved second velocity component. These MIR absorption lines likely probe the molecular material in two edge-on disks, supporting the scenario that NGC 7538 IRS 1 consists of multiple protostars. We provide an updated line list for the torsional band of CH 3 OH, which was generated from lab work and model calculations. This discovery and the updated line list will enable the search for CH 3 OH in JWST/MIRI spectra.

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Publication Details

Journal
The Astrophysical Journal Letters
Published
2025-08-20
DOI
https://doi.org/10.3847/2041-8213/adf632
Primary Topic
Spectroscopy and Laser Applications
Type
article
Field-Weighted Citation Impact
0.00

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article

The Discovery of 25 μm Interstellar Methanol

William D. Vacca, Clara Sousa‐Silva, Edward Montiel, Xinchuan Huang et al.
The Astrophysical Journal Letters
Spectroscopy and Laser Applications
article

The Discovery of 25 μm Interstellar Methanol

William D. Vacca, Clara Sousa‐Silva, Edward Montiel, Xinchuan Huang, C. A. Nixon, Jason Dittmann, G. M. Harper, J. P. Fonfría, Naseem Rangwala, Keeyoon Sung, Sean W. J. Colgan, Sarah Nickerson, Valentin J. M. Le Gouellec, A. G. G. M. Tielens, K. E. Kraemer, Curtis DeWitt, Maisie Rashman, Jialu Li
article en

Abstract

Abstract We present the first astrophysical detection of methanol (CH 3 OH) in the torsional band near 25 μ m. Using high-resolution mid-infrared (MIR) spectroscopy, we identified over 70 gas-phase CH 3 OH absorption lines between 20 and 28 μ m toward the massive protostar NGC 7538 IRS 1 with the Stratospheric Observatory for Infrared Astronomy/Echelon-Cross-Echelle Spectrograph. We derive a temperature of 180 K and a total column density of 2 × 10 17 cm −2 , comparable to submillimeter measurements. Complementary analysis of acetylene (C 2 H 2 ) absorption lines is also included. Both CH 3 OH and C 2 H 2 reveal an unresolved second velocity component. These MIR absorption lines likely probe the molecular material in two edge-on disks, supporting the scenario that NGC 7538 IRS 1 consists of multiple protostars. We provide an updated line list for the torsional band of CH 3 OH, which was generated from lab work and model calculations. This discovery and the updated line list will enable the search for CH 3 OH in JWST/MIRI spectra.

The Astrophysical Journal LettersVol. 989(2)
National Aeronautics and Space Administration, California Institute of Technology, Universities Space Research Association, Nuclear Safety and Security Commission, Universität Stuttgart, Jet Propulsion Laboratory
Openalex Percentile: Top 81%
Spectroscopy and Laser Applications
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