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

Published online by Cambridge University Press:  16 July 2018

Fabrizio Massi ,
Luca Moscadelli ,
Carmelo Arcidiacono  and
Francesca Bacciotti
Fabrizio Massi
Affiliation:
INAF - Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, I–50125, Firenze, Italy email: [email protected], [email protected], [email protected]
Luca Moscadelli
Affiliation:
INAF - Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, I–50125, Firenze, Italy email: [email protected], [email protected], [email protected]
Carmelo Arcidiacono
Affiliation:
INAF - Osservatorio Astronomico di Bologna, Via Piero Gobetti, 93/3, I–40129 Bologna, Italy email: [email protected]
Francesca Bacciotti
Affiliation:
INAF - Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, I–50125, Firenze, Italy email: [email protected], [email protected], [email protected]
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Abstract

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Whether 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.

Keywords

masersstars: formationinfrared: stars
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 13 , Symposium S336: Astrophysical Masers: Unlocking the Mysteries of the Universe , September 2017 , pp. 289 - 290
Copyright
Copyright © International Astronomical Union 2018 

References

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