Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/27280
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Hause, Connor | en_US |
dc.contributor.author | Sion, Edward M. | en_US |
dc.contributor.author | Godon, Patrick | en_US |
dc.contributor.author | Gänsicke, Boris T. | en_US |
dc.contributor.author | Szkody, Paula | en_US |
dc.contributor.author | DE MARTINO, Domitilla | en_US |
dc.contributor.author | Pala, Anna | en_US |
dc.date.accessioned | 2020-09-10T10:32:15Z | - |
dc.date.available | 2020-09-10T10:32:15Z | - |
dc.date.issued | 2017 | en_US |
dc.identifier.issn | 0004-6256 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/27280 | - |
dc.description.abstract | We present a synthetic spectral analysis of the HST COS spectrum of the U Geminorum-type dwarf nova CW Mon, taken during quiescence as part of our COS survey of accreting white dwarfs (WDs) in Cataclysmic Variables. We use a synthetic photosphere and optically thick accretion disk spectra to model the COS spectrum as well as archival IUE spectra obtained decades ago, when the system was in an even deeper quiescent state. Assuming a reddening of E(B-V) = 0.06, an inclination of 60° (CW Mon has eclipses of the accretion disk), and a WD mass of 0.8 {M}<SUB>☉ </SUB>, our results indicate the presence of a 22-27,000 K WD and a low mass accretion rate \dot{M}≲ {10}<SUP>-10</SUP> {M}<SUB>☉ </SUB> {{yr}}<SUP>-1</SUP>, for a derived distance of ∼200 to ∼300 pc. <P />Based on observations made with the NASA-Hubble Space Telescope. | en_US |
dc.language.iso | eng | en_US |
dc.title | Hubble COS Spectroscopy of the Dwarf Nova CW Mon: The White Dwarf in Quiescence? | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.3847/1538-3881/aa774c | en_US |
dc.identifier.scopus | 2-s2.0-85024927026 | en_US |
dc.identifier.isi | 000406855900002 | en_US |
dc.identifier.url | https://iopscience.iop.org/article/10.3847/1538-3881/aa774c | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 154 | en_US |
dc.relation.issue | 2 | en_US |
dc.relation.numberofpages | 6 | en_US |
dc.relation.article | 48 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.numberofauthors | 7 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | USA | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | THE ASTRONOMICAL JOURNAL | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2017AJ....154...48H | en_US |
dc.relation.fund | H2020 | 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 | 0004-6256 | - |
crisitem.journal.ance | E016224 | - |
Appears in Collections: | 1.01 Articoli in rivista |
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File | Description | Size | Format | |
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Hause_2017_AJ_154_48.pdf | Pdf editoriale | 668.15 kB | Adobe PDF | View/Open |
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