{"doi":"10.1051/0004-6361/201730858","title":"Zeeman effect in sulfur monoxide","abstract":null,"journal":"Astronomy & Astrophysics","year":2017,"id":677174,"datarank":0.31191623125197543,"base_score":2.0794415416798357,"endowment":2.0794415416798357,"self_citation_contribution":0.31191623125197543,"citation_network_contribution":0.0,"self_endowment_contribution":0.31191623125197543,"citer_contribution":0.0,"corpus_percentile":null,"corpus_rank":null,"citation_count":7,"citer_count":0,"citers_with_citation_signal":0,"citers_with_endowment":0,"datacite_reuse_total":0,"is_dataset":false,"is_dataset_confidence":null,"is_data_producer":false,"deposit_databanks":null,"is_oa":false,"file_count":0,"downloads":0,"has_version_chain":false,"published_date":null,"fair_score":null,"fair_percentile":null,"algorithm_id":"datarank_citation_only_1hop_v6","ranking_scope":"data_only","authors":[{"id":1769347,"name":"Valerio Lattanzi","orcid":null,"position":1,"is_corresponding":false},{"id":1769349,"name":"Sonia Coriani","orcid":null,"position":2,"is_corresponding":false},{"id":1565049,"name":"Jürgen Gauss","orcid":null,"position":3,"is_corresponding":false},{"id":1769353,"name":"Claudio Codella","orcid":null,"position":4,"is_corresponding":false},{"id":1769354,"name":"Andrés Asensio Ramos","orcid":null,"position":5,"is_corresponding":false},{"id":1769355,"name":"José Cernicharo","orcid":null,"position":6,"is_corresponding":false},{"id":1769356,"name":"Cristina Puzzarini","orcid":"0000-0002-2395-8532","position":7,"is_corresponding":false},{"id":1769346,"name":"Gabriele Cazzoli","orcid":null,"position":0,"is_corresponding":false}],"reference_count":0,"raw_metadata":{"has_enrichment":true,"resolved":true,"title":"Zeeman effect in sulfur monoxide","abstract":"CONTEXT: Magnetic fields play a fundamental role in star formation processes and the best method to evaluate their intensity is to measure the Zeeman effect of atomic and molecular lines. However, a direct measurement of the Zeeman spectral pattern from interstellar molecular species is challenging due to the high sensitivity and high spectral resolution required. So far, the Zeeman effect has been detected unambiguously in star forming regions for very few non-masing species, such as OH and CN. AIMS: We decided to investigate the suitability of sulfur monoxide (SO), which is one of the most abundant species in star forming regions, for probing the intensity of magnetic fields via the Zeeman effect. METHODS: has been carried out. RESULTS: = 2, 1 ← 1, 0 (329.4 GHz). Our investigation supports SO as a good candidate for probing magnetic fields in high-density star forming regions.","is_dataset_classified":null,"base_score":2.0794415416798357,"endowment":2.0794415416798357,"datacite_reuse_total":0,"file_count":0,"downloads":0,"views":0,"has_version_chain":false,"is_dataset":false,"is_oa":false,"pmid":"29151607","pmcid":"PMC5693346","openalex_id":"https://openalex.org/W2615906336","authors":[],"funders":[{"funder_name":"European Research Council","grant_id":"610256","title":null}],"total_grants":1,"fwci":0.4158,"citation_percentile":0.58109396,"influential_citations":0,"citation_trend":[{"year":2018,"count":1},{"year":2019,"count":1},{"year":2020,"count":1},{"year":2022,"count":2},{"year":2023,"count":1},{"year":2026,"count":1}],"oa_status":"bronze","license":"other-oa","oa_locations":[{"url":"https://www.aanda.org/articles/aa/pdf/2017/09/aa30858-17.pdf","host_type":"journal"},{"url":"https://www.aanda.org/articles/aa/pdf/2017/09/aa30858-17.pdf","host_type":"publisher"},{"url":"http://www.aanda.org/10.1051/0004-6361/201730858/pdf","host_type":"publisher"},{"url":"https://doi.org/10.1051/0004-6361/201730858","host_type":"journal"},{"url":"https://pubmed.ncbi.nlm.nih.gov/29151607","host_type":"repository"},{"url":"https://pure.au.dk/portal/en/publications/0ed62c5d-6379-4838-9899-146052dab1b7","host_type":""},{"url":"https://www.aanda.org/10.1051/0004-6361/201730858/pdf","host_type":"repository"},{"url":"https://www.ncbi.nlm.nih.gov/pmc/articles/5693346","host_type":"repository"},{"url":"http://hdl.handle.net/11585/624727","host_type":"repository"},{"url":"http://hdl.handle.net/10261/188167","host_type":"repository"},{"url":"https://orbit.dtu.dk/en/publications/97fe61c8-4cbb-45f7-b8d5-08ef1855d976","host_type":"repository"},{"url":"http://hdl.handle.net/11858/00-001M-0000-002E-3830-7","host_type":"repository"}],"fields_of_study":["Atmospheric Ozone and Climate","Molecular Spectroscopy and Structure","Spectroscopy and Laser Applications"],"mesh_terms":[],"keywords":["Physics","Astrophysics","Carbon monoxide","Sulfur","Monoxide","Zeeman effect","Astronomy","Magnetic field","Inorganic chemistry","Chemistry","Quantum mechanics","Magnetic fields","Molecular Data","Ism: Molecules","Methods: Data Analysis","Methods: Laboratory: Molecular"],"sdg_mappings":[{"sdg_number":0,"sdg_label":"Life below water"}],"linked_datasets":[],"clinical_trials":[],"software_tools":[],"database_accessions":[],"source":"live","citation_network_status":"fetched"},"created_at":"2026-08-17T03:43:48.786966Z","pmid":null,"pmcid":null,"fwci":null,"citation_percentile":null,"influential_citations":0,"oa_status":null,"license":null,"views":0,"total_file_size_bytes":0,"version_count":0,"fair_f":null,"fair_a":null,"fair_i":null,"fair_r":null,"fair_zscore":null,"fair_rationale":null,"fair_model":null,"fair_agent_version":null,"fair_fulltext_source":null,"fair_has_llm":null,"fair_computed_at":null,"clinical_trials":[],"software_tools":[],"db_accessions":[],"linked_datasets":[],"topics":[]}