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dc.contributor.authorGoedhart, S.en_US
dc.contributor.authorLanga, M.C.en_US
dc.contributor.authorVan der Walt, D.J.
dc.contributor.authorGaylard, M.J.
dc.date.accessioned2010-08-04T15:37:45Z
dc.date.available2010-08-04T15:37:45Z
dc.date.issued2009en_US
dc.identifier.citationGoedhart, S. et al. 2009. Short-period variability in the Class II methanol maser source G12.89+0.49 (IRAS 18089-1732). Monthly notices of the Royal Astronomical Society, 398(2):995-1010. [https://doi.org/10.1111/j.1365-2966.2009.15176.x]en_US
dc.identifier.issn0035-8711
dc.identifier.issn1365-2966(Online)
dc.identifier.urihttp://hdl.handle.net/10394/3535
dc.identifier.urihttps://doi.org/10.1111/j.1365-2966.2009.15176.x
dc.identifier.urihttps://academic.oup.com/mnras/article-lookup/doi/10.1111/j.1365-2966.2009.15176.x
dc.description.abstractTime series are presented for the Class II methanol maser source G12.89+0.49, which has been monitored for nine years at the Hartebeesthoek Radio Astronomy Observatory. The 12.2 and 6.7 GHz methanol masers were seen to exhibit rapid, correlated variations on time-scales of less than a month. Daily monitoring has revealed that the variations have a periodic component with a period of 29.5 d. The period seems to be stable over the 110 cycles spanned by the time series. There are variations from cycle to cycle, with the peak of the flare occurring anywhere within an 11 d window, but the minima occur at the same phase of the cycle. Time delays of up to 5.7 d are seen between spectral features at 6.7 GHz and a delay of 1.1 d is seen between the dominant 12.2 GHz spectral feature and its 6.7 GHz counterpart
dc.publisherOxford Univ Press
dc.subjectRadio lines: ISM
dc.subjectH ii regions
dc.subjectISM: clouds
dc.subjectMasers
dc.subjectStars: formation
dc.titleShort-period variability in the Class II methanol maser source G12.89+0.49 (IRAS 18089-1732)en_US
dc.contributor.researchID11699612 - Goedhart, Sharmila
dc.contributor.researchID10060499 - Van der Walt, Diederick Johannes


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