Abstract
We have used the IRAM Plateau de Bure Interferometer to observe the ground state and vibrationally excited lines of methyl cyanide towards the UC HIi region G31.41+0.31. We also obtained a map of the continuum emission at a frequency of 110 GHz. We detect a hot molecular core in the emission both of methyl cyanide and of the 110 GHz continuum. We estimate a temperature of 200 K and a mass of 1000 M⊙ for this compact massive region. We also detect a velocity gradient or shift across the methyl cyanide core whose origin could be due to rotation.
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© 1996 Springer-Verlag
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Cesaroni, R., Olmi, L., Walmsley, C.M., Churchwell, E., Hofner, P. (1996). A massive “core” associated with the UC HIi region G31.41+0.31. In: Beckwith, S., Staude, J., Quetz, A., Natta, A. (eds) Disks and Outflows Around Young Stars. Lecture Notes in Physics, vol 465. Springer, Berlin, Heidelberg. https://doi.org/10.1007/BFb0102636
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DOI: https://doi.org/10.1007/BFb0102636
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