Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/29208
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Toloza, Odette | en_US |
dc.contributor.author | Breedt, Elme | en_US |
dc.contributor.author | DE MARTINO, Domitilla | en_US |
dc.contributor.author | Drake, Jeremy | en_US |
dc.contributor.author | Gansicke, Boris | en_US |
dc.contributor.author | Green, Matthew | en_US |
dc.contributor.author | Ederoclite, Alessandro | en_US |
dc.contributor.author | Jennifer, Johnson | en_US |
dc.contributor.author | Juna, Kollmeier | en_US |
dc.contributor.author | Knigge, Christian | en_US |
dc.contributor.author | Kupfer, Thomas | en_US |
dc.contributor.author | Long, Knox | en_US |
dc.contributor.author | Marsh, Thomas | en_US |
dc.contributor.author | Pala, Anna | en_US |
dc.contributor.author | Parsons, Steven | en_US |
dc.contributor.author | Prince, Tom | en_US |
dc.contributor.author | Raddi, Roberto | en_US |
dc.contributor.author | Rebassa-Manserga, Alberto | en_US |
dc.contributor.author | Rodriguez-Gil, Pablo | en_US |
dc.contributor.author | Scaringi, Simone | en_US |
dc.contributor.author | Schmidtobreick, Linda | en_US |
dc.contributor.author | Schreiber, Matthias | en_US |
dc.contributor.author | Schwope, Axel | en_US |
dc.contributor.author | Shen, Ken | en_US |
dc.contributor.author | Steeghs, Danny | en_US |
dc.contributor.author | Szkody, Paula | en_US |
dc.contributor.author | Tappert, Claus | en_US |
dc.contributor.author | Toonen, Silvia | en_US |
dc.contributor.author | Townsley, Dean | en_US |
dc.contributor.author | Zorotovic, Monica | en_US |
dc.date.accessioned | 2020-12-28T12:18:44Z | - |
dc.date.available | 2020-12-28T12:18:44Z | - |
dc.date.issued | 2019 | en_US |
dc.identifier.issn | 2330-9458 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/29208 | - |
dc.description.abstract | In this white paper we stressed the importance of ultraviolet (high- resolution) and optical (low- and high-) spectroscopy to understand of evolution of close binaries that contain white dwarfs which lead to a variety of outcomes. | en_US |
dc.language.iso | eng | en_US |
dc.title | Understanding the evolution of close white dwarf binaries | en_US |
dc.type | Article | - |
dc.identifier.url | https://baas.aas.org/pub/2020n3i168/release/1 | en_US |
dc.identifier.url | https://arxiv.org/pdf/1903.04612.pdf | en_US |
dc.relation.medium | ELETTRONICO | en_US |
dc.relation.volume | 51 | en_US |
dc.relation.issue | 3 | en_US |
dc.relation.firstpage | 168 | en_US |
dc.relation.numberofpages | 8 | en_US |
dc.relation.article | 168 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | USA | en_US |
dc.contributor.country | GBR | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | BULLETIN OF THE AMERICAN ASTRONOMICAL SOCIETY | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2019BAAS...51c.168T | en_US |
dc.relation.ercsector | ERC sectors::Physical Sciences and Engineering | 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. Capodimonte | - |
crisitem.author.orcid | 0000-0002-5069-4202 | - |
crisitem.journal.journalissn | 2330-9458 | - |
crisitem.journal.ance | E224837 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
71598543863112.pdf | postprint | 334.66 kB | Adobe PDF | View/Open |
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