Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/24687
DC Field | Value | Language |
---|---|---|
dc.contributor.author | BELTRAN SOROLLA, MARIA TERESA | en_US |
dc.contributor.author | de Wit, W. J. | en_US |
dc.date.accessioned | 2020-05-11T12:16:09Z | - |
dc.date.available | 2020-05-11T12:16:09Z | - |
dc.date.issued | 2016 | en_US |
dc.identifier.issn | 0935-4956 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/24687 | - |
dc.description.abstract | An observational review is provided of the properties of accretion disks around young stars. It concerns the primordial disks of intermediate- and high-mass young stellar objects in embedded and optically revealed phases. The properties were derived from spatially resolved observations and, therefore, predominantly obtained with interferometric means, either in the radio/(sub)millimeter or in the optical/infrared wavelength regions. We make summaries and comparisons of the physical properties, kinematics, and dynamics of these circumstellar structures and delineate trends where possible. Amongst others, we report on a quadratic trend of mass accretion rates with mass from T Tauri stars to the highest mass young stellar objects and on the systematic difference in mass infall and accretion rates. | en_US |
dc.language.iso | eng | en_US |
dc.title | Accretion disks in luminous young stellar objects | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1007/s00159-015-0089-z | en_US |
dc.identifier.scopus | 2-s2.0-84954451489 | en_US |
dc.identifier.isi | 000368075900002 | en_US |
dc.identifier.url | https://link.springer.com/article/10.1007/s00159-015-0089-z | en_US |
dc.relation.medium | ELETTRONICO | en_US |
dc.relation.volume | 24 | en_US |
dc.relation.firstpage | 6 | en_US |
dc.relation.numberofpages | 71 | en_US |
dc.type.referee | REF_2 | en_US |
dc.description.international | sì | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | THE ASTRONOMY AND ASTROPHYSICS REVIEW | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2016A&ARv..24....6B | en_US |
dc.relation.ercsector | ERC sectors::Physical Sciences and Engineering::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation::PE9_4 Formation of stars and planets | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | en_US |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.openairetype | Article | - |
item.languageiso639-1 | en | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | O.A. Arcetri | - |
crisitem.author.orcid | 0000-0003-3315-5626 | - |
crisitem.journal.journalissn | 0935-4956 | - |
crisitem.journal.ance | E016242 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
Beltran-deWit-2016.pdf | preprint | 2.86 MB | Adobe PDF | View/Open |
Beltrán-Wit2016.pdf | Pdf editoriale | 3.22 MB | Adobe PDF | View/Open |
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