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dc.contributor.authorMacleod, G.C.
dc.contributor.authorChibueze, J.O.
dc.contributor.authorSugiyama, K.
dc.contributor.authorHunter, T.R.
dc.contributor.authorQuick, J.
dc.date.accessioned2019-11-06T09:21:06Z
dc.date.available2019-11-06T09:21:06Z
dc.date.issued2019
dc.identifier.citationMacLeod, G.C. et al. 2019. Detection of new methanol maser transitions associated with G358.93−0.03. Monthly notices of the Royal Astronomical Society, 489(3):3981-3989. [https://doi.org/10.1093/mnras/stz2417]en_US
dc.identifier.issn0035-8711
dc.identifier.issn1365-2966 (Online)
dc.identifier.urihttp://hdl.handle.net/10394/33553
dc.identifier.urihttps://academic.oup.com/mnras/article-pdf/489/3/3981/30040623/stz2417.pdf
dc.identifier.urihttps://doi.org/10.1093/mnras/stz2417
dc.description.abstractWe report the detection of new 12.178, 12.229, 20.347, and 23.121 GHz methanol masers in the massive star-forming region G358.93−0.03, which are flaring on similarly short time-scales (days) as the 6.668 GHz methanol masers also associated with this source. The brightest 12.178 GHz channel increased by a factor of over 700 in just 50 d. The masers found in the 12.229 and 20.347 GHz methanol transitions are the first ever reported and this is only the fourth object to exhibit associated 23.121 GHz methanol masers. The 12.178 GHz methanol maser emission appears to have a higher flux density than that of the 6.668 GHz emission, which is unusual. No associated near-infrared flare counterpart was found, suggesting that the energy source of the flare is deeply embeddeden_US
dc.language.isoenen_US
dc.publisherOxford Univ Pressen_US
dc.subjectMasersen_US
dc.subjectStars: formationen_US
dc.subjectStars: protostarsen_US
dc.subjectISM: individual objects: MMB G358.931-0.030en_US
dc.subjectISM: moleculesen_US
dc.subjectRadio lines: ISMen_US
dc.titleDetection of new methanol maser transitions associated with G358.93−0.03en_US
dc.typeArticleen_US
dc.contributor.researchID29697492 - Chibueze, James Okwe


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