{ "abstract": "Context . Methanol is a complex organic molecule detected in both ice and gas toward star-forming regions. Due to its high abundance, its rarer isotopologues, including the deuterated ones, are also commonly detected. Measurements of deuteration can provide key constraints on the formation and evolution of molecules during the formation of stars and planets. It is not clear how the methanol deuteration varies between star-forming regions. Thanks to several recent spectroscopic studies, it is now possible to precisely derive the column densities of five deuterated isotopologues of methanol.\n\nAims . Our aim is to determine the column density and deuterium fractionation of methanol in the low-mass protostar BHR71-IRS1.\n\nMethods . We analyzed data from a large spectral survey of BHR71-IRS1 carried out as part of the ALMA Large Program Complex Organic Molecules in Protostars with ALMA Spectral Surveys (COMPASS). We used the CASSIS software to identify the lines of the methanol isotopologues and constrain their column densities under the assumption of local thermodynamic equilibrium.\n\nResults . We detected CH ₃ OH, ¹³ CH ₃ OH, CH ₃ ¹⁸ OH, CH ₃ OD, CH ₂ DOH, CHD ₂ OH, and CD ₃ OH at the continuum peak position. In addition, CH ₃ ¹⁷ OH is tentatively detected, while CD ₃ OD is not detected, although a few faint lines (≲3 σ ) could be present toward a position redshifted from the continuum peak. The column densities of the main isotopologue obtained from ¹³ CH ₃ OH and CH ₃ ¹⁸ OH are consistent, assuming nominal ¹² C/ ¹³ C and ¹⁶ O/ ¹⁸ O ratios of 68 and 557, respectively. The CH ₂ DOH/CH ₃ OD column density ratio is equal to 7 ± 2. The statistically corrected D/H ratio is higher for CH ₂ DOH (1.9 ± 0.6%) than for CH ₃ OD (0.8 ± 0.2%). The level of deuteration after statistical correction increases with the number of D atoms in the methyl group, reaching 23 ± 5% for CD ₃ OH/CH ₃ OH.\n\nConclusions . These trends are similar to other low-mass protostars such as IRAS 16293–2422 and HOPS 373SW, but seem to differ from the eruptive young star V883-Ori. Similar studies with comparable datasets will be carried out for the other COMPASS sources to determine if factors such as environmental conditions and evolutionary states impact the deuteration of methanol.", "abstract_shown": true, "affiliations": [ "Institut de Recherche en Astrophysique et Planétologie, Université de Toulouse, CNRS, CNES", "Niels Bohr Institute, University of Copenhagen", "Physikalisch-Meteorologisches Observatorium Davos und Weltstrahlungszentrum (PMOD/WRC)", "Department of Chemistry, Biochemistry and Pharmaceutical Sciences (DCBP), Universität Bern", "Department of Physics and Astronomy, Seoul National University", "National Radio Astronomy Observatory", "Institute of Astronomy, Department of Physics, National Tsinghua University", "Univ. Grenoble Alpes, CNRS, IPAG", "Max-Planck-Institut für Radioastronomie", "RIKEN, Star and Planet Formation Laboratory, RIKEN Pioneering Research Institute, Wako-shi", "Purdue University", "Konkoly Observatory, HUN-REN Research Centre for Astronomy and Earth Sciences, MTA Centre of Excellence", "Institute of Physics and Astronomy, ELTE Eötvös Loránd University", "Max-Planck-Institut für Astronomie", "Department of Chemistry, Massachusetts Institute of Technology", "European Southern Observatory, European Southern Observatory", "Max-Planck-Institut für extraterrestrische Physik", "Department of Astronomy, University of Virginia", "Korea Astronomy and Space Science Institute", "UC Berkeley, Department of Chemistry", "Faculty of Aerospace Engineering, Delft University of Technology, Delft", "Institute of Astronomy and Astrophysics, Academia Sinica" ], "article_type": null, "arxiv": null, "author_total": 29, "authors": [ { "affs": [ 0 ], "name": "A. Coutens", "orcid": "0000-0003-1805-3920" }, { "affs": [ 0 ], "name": "F. Cruz-Sáenz de Miera", "orcid": "0000-0002-4283-2185" }, { "affs": [ 1 ], "name": "J. K. Jørgensen", "orcid": "0000-0001-9133-8047" }, { "affs": [ 2, 3 ], "name": "M. N. Drozdovskaya", "orcid": "0000-0001-7479-4948" }, { "affs": [ 4 ], "name": "J.-E. Lee", "orcid": "0000-0003-3119-2087" }, { "affs": [ 5 ], "name": "A. L. Plunkett", "orcid": "0000-0002-9912-5705" }, { "affs": [ 6 ], "name": "D. Harsono", "orcid": "0000-0001-6307-4195" }, { "affs": [ 7 ], "name": "S. Maret", "orcid": "0000-0003-1104-4554" }, { "affs": [ 8 ], "name": "A. Belloche", "orcid": "0000-0003-0046-6217" }, { "affs": [ 9 ], "name": "J. Ferrer Asensio", "orcid": "0000-0002-1095-9368" }, { "affs": [ 10 ], "name": "M. L. R. van’t Hoff", "orcid": "0000-0002-2555-9869" }, { "affs": [ 4 ], "name": "J.-H. Jeong", "orcid": "0009-0005-6319-8485" }, { "affs": [ 11, 12, 13 ], "name": "Á. Kóspál", "orcid": "0000-0001-7157-6275" }, { "affs": [ 14, 5 ], "name": "B. A. McGuire", "orcid": "0000-0003-1254-4817" }, { "affs": [ 15 ], "name": "P. Nazari", "orcid": "0000-0002-4448-3871" }, { "affs": [ 16 ], "name": "S. Spezzano", "orcid": "0000-0002-6787-5245" }, { "affs": [ 17 ], "name": "Z. Telkamp", "orcid": "0000-0001-6465-9590" }, { "affs": [ 9 ], "name": "Y.-L. Yang", "orcid": "0000-0001-8227-2816" }, { "affs": [ 4, 18 ], "name": "H.-S. Yun", "orcid": "0000-0001-6842-1555" }, { "affs": [ 9 ], "name": "S. Zeng", "orcid": "0000-0003-3721-374X" }, { "affs": [ 0 ], "name": "A. Andreu", "orcid": "0009-0002-3985-9253" }, { "affs": [ 19 ], "name": "J. Bergner", "orcid": "0000-0002-8716-0482" }, { "affs": [ 4 ], "name": "C.-H. Kim", "orcid": "0000-0002-2523-3762" }, { "affs": [ 20 ], "name": "N. F. W. Ligterink", "orcid": "0000-0002-8385-9149" }, { "affs": [ 16 ], "name": "Y. Lin", "orcid": "0000-0001-9299-5479" }, { "affs": [ 21 ], "name": "S.-Y. Liu" }, { "affs": [ 1 ], "name": "M. Lützen", "orcid": "0009-0001-5802-0974" }, { "affs": [ 0 ], "name": "P. Marchand", "orcid": "0000-0002-4577-8292" }, { "affs": [ 17 ], "name": "M. Rao", "orcid": "0000-0003-0551-4898" } ], "bibtex": "https://research.draconitic.com/paper/3as20ez28z4jp.bib", "cited_by": 4, "doi": "10.1051/0004-6361/202558733", "fulltext_url": null, "id": "3as20ez28z4jp", "issns": [ "0004-6361", "1432-0746" ], "landing_url": "https://www.aanda.org/10.1051/0004-6361/202558733", "language": null, "licence": "CC-BY-4.0", "licence_label": "CC BY 4.0", "licence_source": "article", "licence_url": "https://creativecommons.org/licenses/by/4.0", "metadata_licence": null, "native_subjects": [ [ "openalex", "3103|Astrophysics and Star Formation Studies" ] ], "openalex": "W7220835312", "pdf_url": null, "pmcid": null, "pmid": null, "published": "2026-10-07", "publisher": "EDP Sciences", "ris": "https://research.draconitic.com/paper/3as20ez28z4jp.ris", "sources": [ { "first_seen": "2026-10-30T12:18:18Z", "native_id": "10.1051/0004-6361/202558733", "source": "crossref", "url": "https://www.aanda.org/10.1051/0004-6361/202558733" } ], "subjects": [ { "field": "astronomy", "origin": "openalex:3103|Astrophysics and Star Formation Studies", "subfield": "stellar" } ], "title": "Complex Organic Molecules in Protostars with ALMA Spectral Surveys (COMPASS)", "title_text": "Complex Organic Molecules in Protostars with ALMA Spectral Surveys (COMPASS)", "type": "peer-reviewed", "updated_at": "2026-10-30T12:18:18Z", "url": "https://research.draconitic.com/paper/3as20ez28z4jp", "venue": "Astronomy & Astrophysics", "versions": [ { "doi": "10.48550/arxiv.2610.07463", "pid": "bvkz0hx6cvbr8", "relation": "preprint", "title": "Complex Organic Molecules in Protostars with ALMA Spectral Surveys (COMPASS) III. CH$_3$OH isotopic fractionation in the low-mass protostar BHR71-IRS1", "venue": "arXiv" } ] }