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Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S242(3), p. 135-139, 2007

DOI: 10.1017/s1743921307012690

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Massive star-formation in G24.78+0.08 studied by means of maser VLBI and thermal interferometric observations

Journal article published in 2007 by L. Moscadelli, C. Goddi, R. Cesaroni ORCID, M. T. Beltràn
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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Abstract

AbstractThis work presents the results of VLBI observations of 6.7 GHz methanol and 22.2 GHz water masers towards the mm core A in the massive star-forming region G24.78+0.08. Comparing the maser with previous millimeter interferometric and recent continuum VLA observations, the physical properties and the gas kinematics of the G24 A core on linear scales from ~100 AU to ~0.1 pc are determined.

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