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Discovery of the Zeeman Effect in the 36 and 44 GHz Class I Methanol Maser Lines with the EVLA (PUB-152)

PUB-152 · 2010 · Proceedings of Science1

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  1. The observations were carried out with the Expanded Very Large Array (EVLA) toward the star-forming regions M8E (at 36 GHz) and OMC-2 (at 44 GHz). Archived source retained by Resource Map maintainers. View current source