OLMI, LUCALUCAOLMIAraya, Esteban D.Esteban D.ArayaArmstrong, JasonJasonArmstrong2021-01-262021-01-262018978-11071924541743-9213http://hdl.handle.net/20.500.12386/30004In 2014 we conducted a survey for 6.7 GHz methanol masers with the Arecibo Tele- scope toward far infrared sources selected from the Hi-GAL catalog of massive cores. We found a number of sources with weak 6.7GHz methanol masers, possibly indicating regions in early stages of star formation. Here we describe the results of follow-up observations that were con- ducted with the Very Large Array in New Mexico to characterize this new population of “weak” 6.7 GHz methanol masers.STAMPAenVLA Observations of a Sample of Low-Brightness 6.7 GHz Methanol MasersConference paper10.1017/S1743921318000807https://www.cambridge.org/core/journals/proceedings-of-the-international-astronomical-union/article/vla-observations-of-a-sample-of-lowbrightness-67-ghz-methanol-masers/04AA9F611E0AF9A4F73A86128AF765182018IAUS..336..311OFIS/05 - ASTRONOMIA E ASTROFISICA