The innermost regions of massive protostars traced by masers, high-resolution radio continuum, and near-infrared imaging
Date Issued
2018
Author(s)
Abstract
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.
Coverage
Astrophysical Masers: Unlocking the Mysteries of the Universe
All editors
Tarchi, Andrea; Reid, Mark J.; Castangia, Paola
Volume
336
Start page
289
Conferenece
Astrophysical Masers: Unlocking the Mysteries of the Universe
Conferenece place
Cagliari, Italy
Conferenece date
4-8 September, 2017
Issn Identifier
1743-9213
Ads BibCode
2018IAUS..336..289M
Rights
open.access
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