Matches in SemOpenAlex for { <https://semopenalex.org/work/W4429214> ?p ?o ?g. }
Showing items 1 to 64 of
64
with 100 items per page.
- W4429214 endingPage "647" @default.
- W4429214 startingPage "647" @default.
- W4429214 abstract "Ultraviolet spectroscopic observations made with the Copernicus and IUE spacecraft have been analyzed. The observations represent a collaborative effort with G. J. Peters. Observational evidence supporting the existence of a turbulent accretion layer has been discussed earlier by Peters. Ionization equilibrium calculations suggest the following physical conditions in the layer: T ~ 125000 K°, N e ~ 109 cm -3 ; composition: Nitrogen rich, carbon poor. Observations also show the region to be turbulent and not co-rotating with the accreting star. We conclude that the region is formed by new material arriving from the secondary and that the accretion process is turbulent." @default.
- W4429214 created "2016-06-24" @default.
- W4429214 creator A5065409834 @default.
- W4429214 date "1983-01-01" @default.
- W4429214 modified "2023-10-16" @default.
- W4429214 title "UV Observations of Close Binary Stars" @default.
- W4429214 doi "https://doi.org/10.1017/s1539299600005724" @default.
- W4429214 hasPublicationYear "1983" @default.
- W4429214 type Work @default.
- W4429214 sameAs 4429214 @default.
- W4429214 citedByCount "0" @default.
- W4429214 crossrefType "journal-article" @default.
- W4429214 hasAuthorship W4429214A5065409834 @default.
- W4429214 hasBestOaLocation W44292141 @default.
- W4429214 hasConcept C121332964 @default.
- W4429214 hasConcept C1276947 @default.
- W4429214 hasConcept C145148216 @default.
- W4429214 hasConcept C150846664 @default.
- W4429214 hasConcept C153294291 @default.
- W4429214 hasConcept C193786831 @default.
- W4429214 hasConcept C196558001 @default.
- W4429214 hasConcept C198291218 @default.
- W4429214 hasConcept C2776401274 @default.
- W4429214 hasConcept C2776798109 @default.
- W4429214 hasConcept C33923547 @default.
- W4429214 hasConcept C44870925 @default.
- W4429214 hasConcept C48372109 @default.
- W4429214 hasConcept C62520636 @default.
- W4429214 hasConcept C94375191 @default.
- W4429214 hasConceptScore W4429214C121332964 @default.
- W4429214 hasConceptScore W4429214C1276947 @default.
- W4429214 hasConceptScore W4429214C145148216 @default.
- W4429214 hasConceptScore W4429214C150846664 @default.
- W4429214 hasConceptScore W4429214C153294291 @default.
- W4429214 hasConceptScore W4429214C193786831 @default.
- W4429214 hasConceptScore W4429214C196558001 @default.
- W4429214 hasConceptScore W4429214C198291218 @default.
- W4429214 hasConceptScore W4429214C2776401274 @default.
- W4429214 hasConceptScore W4429214C2776798109 @default.
- W4429214 hasConceptScore W4429214C33923547 @default.
- W4429214 hasConceptScore W4429214C44870925 @default.
- W4429214 hasConceptScore W4429214C48372109 @default.
- W4429214 hasConceptScore W4429214C62520636 @default.
- W4429214 hasConceptScore W4429214C94375191 @default.
- W4429214 hasLocation W44292141 @default.
- W4429214 hasOpenAccess W4429214 @default.
- W4429214 hasPrimaryLocation W44292141 @default.
- W4429214 hasRelatedWork W1986109513 @default.
- W4429214 hasRelatedWork W2029125027 @default.
- W4429214 hasRelatedWork W2035372655 @default.
- W4429214 hasRelatedWork W2091176966 @default.
- W4429214 hasRelatedWork W2132853087 @default.
- W4429214 hasRelatedWork W2147774829 @default.
- W4429214 hasRelatedWork W2331477506 @default.
- W4429214 hasRelatedWork W3025583006 @default.
- W4429214 hasRelatedWork W4224438329 @default.
- W4429214 hasRelatedWork W4321442755 @default.
- W4429214 hasVolume "6" @default.
- W4429214 isParatext "false" @default.
- W4429214 isRetracted "false" @default.
- W4429214 magId "4429214" @default.
- W4429214 workType "article" @default.