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Massive star-formation in G24.78+0.08 studied by means of maser VLBI and thermal interferometric observations
Published online by Cambridge University Press: 01 March 2007
Abstract
This 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.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 3 , Symposium S242: Astrophysical Masers and their Environments , March 2007 , pp. 135 - 139
- Copyright
- Copyright © International Astronomical Union 2008