Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/28395
Campo DC | Valore | Lingua |
---|---|---|
dc.contributor.author | Howell, Steve B. | en_US |
dc.contributor.author | MASON, Elena | en_US |
dc.date.accessioned | 2020-11-17T16:51:56Z | - |
dc.date.available | 2020-11-17T16:51:56Z | - |
dc.date.issued | 2018 | en_US |
dc.identifier.issn | 0004-6256 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/28395 | - |
dc.description.abstract | Using a sample of Nova-like stars from the Ritter & Kolb catalog, we examine the relationship between their Gaia-determined absolute magnitude and the inclination of the binary system. Webbink et al. derived a relationship between these two variables that provides a good fit and allows differentiation between \dot{M} (and possibly M _WD) as a function of inclination. We show that the spread in M_V, at a given i, is dominated by the mass-transfer rate with only a small dependence on the white dwarf mass. The validated relation shows that present-day theoretical population studies of cataclysmic variables, as well as model fits to observational data, yield mass-transfer rates and white dwarf masses consistent with the Gaia-derived M _V for the nova-like stars. | en_US |
dc.language.iso | eng | en_US |
dc.title | On the M_V -Inclination Relationship for Nova-like Variables | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.3847/1538-3881/aadd13 | en_US |
dc.identifier.scopus | 2-s2.0-85056699308 | en_US |
dc.identifier.isi | 000447164500008 | en_US |
dc.identifier.url | https://iopscience.iop.org/article/10.3847/1538-3881/aadd13 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 156 | en_US |
dc.relation.issue | 5 | en_US |
dc.relation.firstpage | 198 | 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.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 | 2018AJ....156..198H | 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.cerifentitytype | Publications | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
item.grantfulltext | open | - |
item.languageiso639-1 | en | - |
item.openairetype | Article | - |
crisitem.journal.journalissn | 0004-6256 | - |
crisitem.journal.ance | E016224 | - |
crisitem.author.dept | O.A. Trieste | - |
crisitem.author.orcid | 0000-0003-3877-0484 | - |
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