Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/28089
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Galván-Madrid, R. | en_US |
dc.contributor.author | BELTRAN SOROLLA, MARIA TERESA | en_US |
dc.contributor.author | Ginsburg, A. | en_US |
dc.contributor.author | Carrasco-González, C. | en_US |
dc.contributor.author | Liu, H. B. | en_US |
dc.contributor.author | Rodríguez, L. F. | en_US |
dc.contributor.author | Kurtz, S. | en_US |
dc.date.accessioned | 2020-10-29T15:06:42Z | - |
dc.date.available | 2020-10-29T15:06:42Z | - |
dc.date.issued | 2018 | en_US |
dc.identifier.isbn | 978-1-58381-919-7 | en_US |
dc.identifier.issn | 1050-3390 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/28089 | - |
dc.description.abstract | In this contribution we explore the new science that a next generation Very Large Array (ngVLA) would be able to perform on the topics of the youngest HII regions and (proto)stellar jets. Free-free continuum and radio recombination line (RRL) emission are often the only way of peering into the dense envelopes surrounding (proto)stars of all masses, and trace their initial feedback in the form of 'radio jets', 'hypercompact HII regions', or photoevaporating, partially-ionized flows. Properly disentangling free-free from dust emission is also mandatory in studies of protoplanetary and accretion disks. Current VLA research has reached an impasse in which a population of faint ionized radio sources, probably corresponding to the above mentioned objects, is detected, but their nature is mostly unknown. The ngVLA would allow us to resolve the density structure and kinematics of such sources, revolutionizing our knowledge of star formation across the entire stellar-mass spectrum. | en_US |
dc.language.iso | eng | en_US |
dc.title | Resolving the Structure and Kinematics of the Youngest HII Regions and Radio Jets from Young Stellar Objects | en_US |
dc.type | Conference paper | - |
dc.identifier.url | https://arxiv.org/pdf/1806.10225.pdf | en_US |
dc.identifier.url | http://aspbooks.org/a/volumes/article_details/?paper_id=38691 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 517 | en_US |
dc.relation.firstpage | 309 | en_US |
dc.relation.numberofpages | 12 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.international | sì | en_US |
dc.relation.alleditors | Murphy, E. J. and the ngVLA Science Advisory Council | en_US |
dc.relation.ispartofbook | Science with a Next Generation Very Large Array | en_US |
dc.relation.conferencename | Science with a Next Generation Very Large Array | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.type.miur | 273 Contributo in Atti di convegno | - |
dc.relation.series | ASTRONOMICAL SOCIETY OF THE PACIFIC CONFERENCE SERIES | en_US |
dc.identifier.adsbibcode | 2018ASPC..517..309G | en_US |
dc.relation.ercsector | Scienze Fisiche Settori ERC (ERC) di riferimento::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 | Conference paper | - |
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 | 1050-3390 | - |
crisitem.journal.ance | E210915 | - |
Appears in Collections: | 3.01 Contributi in Atti di convegno |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
1806.10225.pdf | preprint | 3.04 MB | Adobe PDF | View/Open |
ASP517-0309.pdf | Pdf editoriale | 785.45 kB | Adobe PDF | View/Open |
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