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Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S336(13), p. 289-290

DOI: 10.1017/s1743921317011644

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The innermost regions of massive protostars traced by masers, high-resolution radio continuum, and near-infrared imaging

Journal article published in 2017 by Fabrizio Massi, Luca Moscadelli, Carmelo Arcidiacono, Francesca Bacciotti ORCID
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

AbstractWhether high-mass stars (M > 7M⊙) emerge from a scaled-up version of the low-mass star formation scenario, i. e. through disk-mediated accretion, is still debated. We present the first results of an observational programme aimed to map the innermost regions of high-mass stellar objects by combining together high-spatial resolution maser and radio continuum observations, and near-infrared imaging.

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