ATTENZIONE! IL REPOSITORY E’ APERTO ESCLUSIVAMENTE ALL’IMMISSIONE DEI RAPPORTI TECNICI (COLLEZIONE 4.01). NON E’ POSSIBILE INSERIRE PRODOTTI IN TUTTE LE ALTRE COLLEZIONI, A CAUSA DI PROBLEMI TECNICI. THE REPOSITORY IS OPEN EXCLUSIVELY FOR THE SUBMISSION OF TECHNICAL REPORTS (COLLECTION 4.01). SUBMISSIONS TO ALL OTHER COLLECTIONS ARE TEMPORARILY UNAVAILABLE, DUE TO TECHNICAL ISSUES.
 

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

Date Issued
2018
Author(s)
•
•
•
DOI
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
Series
Volume
336
Start page
289
Conferenece
Astrophysical Masers: Unlocking the Mysteries of the Universe
Conferenece place
Cagliari, Italy
Conferenece date
4-8 September, 2017
Uri
Url
Issn Identifier
1743-9213
Ads BibCode
2018IAUS..336..289M
Rights
open.access
File(s)
Loading...
Thumbnail Image
Name

Massi_IAU Symp. 336.pdf

Description
Pdf editoriale
Size

156.73 KB

Format

Adobe PDF

Checksum (MD5)

5e3a0a4342c471ea6c444a44511fefec