FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2019069988> ?p ?o ?g. }

• W2019069988 endingPage "1456" @default.
• W2019069988 startingPage "1446" @default.
• W2019069988 abstract "The theoretical condition for a spectrum line to appear in emission is stated in terms of a parameter which measures the departure from thermodynamic equilibrium of the atmosphere. It is shown briefly that only in very hot stars can emission lines arise in what might be called a normal stellar atmosphere. A simplified method for deriving approximate values of the extent of the atmospheres in Ae and Be stars from the intensities of the Balmer emission lines, originally derived by the authors, is outlined, and some applications are described. A simplified theory of the Balmer decrement in these stars is also discussed. In the second part of the paper a brief summary is given of the different classes of late-type emission objects: long-period variables, RV Tauri and semi-regular variables, population II cepheids (W Virginis variables), cluster-type variables, classical cepheids, stars embedded in dense obscuring clouds (T Tauri stars), flare stars, late-type dwarfs, solar-type stars, some binary systems, R Coronae Borealis stars, explosive dwarf stars (SS Cygni variables). Some physical ideas concerning these are described." @default.
• W2019069988 created "2016-06-24" @default.
• W2019069988 creator A5004282362 @default.
• W2019069988 creator A5090431418 @default.
• W2019069988 date "1956-01-01" @default.
• W2019069988 modified "2023-09-23" @default.
• W2019069988 title "Emission lines and stellar atmospheres" @default.
• W2019069988 cites W1584178682 @default.
• W2019069988 cites W1598439384 @default.
• W2019069988 cites W1965771007 @default.
• W2019069988 cites W1966316584 @default.
• W2019069988 cites W1969390933 @default.
• W2019069988 cites W1970649094 @default.
• W2019069988 cites W1981766493 @default.
• W2019069988 cites W1989405273 @default.
• W2019069988 cites W1996374453 @default.
• W2019069988 cites W2004240670 @default.
• W2019069988 cites W2008733543 @default.
• W2019069988 cites W2012782984 @default.
• W2019069988 cites W2020093265 @default.
• W2019069988 cites W2029400485 @default.
• W2019069988 cites W2030589170 @default.
• W2019069988 cites W2032522986 @default.
• W2019069988 cites W2034716552 @default.
• W2019069988 cites W2036125519 @default.
• W2019069988 cites W2037898733 @default.
• W2019069988 cites W2038545416 @default.
• W2019069988 cites W2046814661 @default.
• W2019069988 cites W2047591989 @default.
• W2019069988 cites W2047999104 @default.
• W2019069988 cites W2050721573 @default.
• W2019069988 cites W2053925147 @default.
• W2019069988 cites W2065553486 @default.
• W2019069988 cites W2067571523 @default.
• W2019069988 cites W2075815645 @default.
• W2019069988 cites W2075953881 @default.
• W2019069988 cites W2084545279 @default.
• W2019069988 cites W2088612131 @default.
• W2019069988 cites W2089100888 @default.
• W2019069988 cites W2092987846 @default.
• W2019069988 cites W2320343809 @default.
• W2019069988 cites W657731508 @default.
• W2019069988 doi "https://doi.org/10.1016/0083-6656(56)90073-3" @default.
• W2019069988 hasPublicationYear "1956" @default.
• W2019069988 type Work @default.
• W2019069988 sameAs 2019069988 @default.
• W2019069988 citedByCount "3" @default.
• W2019069988 crossrefType "journal-article" @default.
• W2019069988 hasAuthorship W2019069988A5004282362 @default.
• W2019069988 hasAuthorship W2019069988A5090431418 @default.
• W2019069988 hasConcept C101638190 @default.
• W2019069988 hasConcept C121332964 @default.
• W2019069988 hasConcept C1276947 @default.
• W2019069988 hasConcept C144024400 @default.
• W2019069988 hasConcept C149923435 @default.
• W2019069988 hasConcept C150739758 @default.
• W2019069988 hasConcept C150846664 @default.
• W2019069988 hasConcept C164546044 @default.
• W2019069988 hasConcept C173220165 @default.
• W2019069988 hasConcept C17352008 @default.
• W2019069988 hasConcept C178075534 @default.
• W2019069988 hasConcept C180690934 @default.
• W2019069988 hasConcept C2908647359 @default.
• W2019069988 hasConcept C44870925 @default.
• W2019069988 hasConcept C4839761 @default.
• W2019069988 hasConcept C80518518 @default.
• W2019069988 hasConcept C96141758 @default.
• W2019069988 hasConceptScore W2019069988C101638190 @default.
• W2019069988 hasConceptScore W2019069988C121332964 @default.
• W2019069988 hasConceptScore W2019069988C1276947 @default.
• W2019069988 hasConceptScore W2019069988C144024400 @default.
• W2019069988 hasConceptScore W2019069988C149923435 @default.
• W2019069988 hasConceptScore W2019069988C150739758 @default.
• W2019069988 hasConceptScore W2019069988C150846664 @default.
• W2019069988 hasConceptScore W2019069988C164546044 @default.
• W2019069988 hasConceptScore W2019069988C173220165 @default.
• W2019069988 hasConceptScore W2019069988C17352008 @default.
• W2019069988 hasConceptScore W2019069988C178075534 @default.
• W2019069988 hasConceptScore W2019069988C180690934 @default.
• W2019069988 hasConceptScore W2019069988C2908647359 @default.
• W2019069988 hasConceptScore W2019069988C44870925 @default.
• W2019069988 hasConceptScore W2019069988C4839761 @default.
• W2019069988 hasConceptScore W2019069988C80518518 @default.
• W2019069988 hasConceptScore W2019069988C96141758 @default.
• W2019069988 hasLocation W20190699881 @default.
• W2019069988 hasOpenAccess W2019069988 @default.
• W2019069988 hasPrimaryLocation W20190699881 @default.
• W2019069988 hasRelatedWork W106919363 @default.
• W2019069988 hasRelatedWork W1520646815 @default.
• W2019069988 hasRelatedWork W1987632441 @default.
• W2019069988 hasRelatedWork W2019069988 @default.
• W2019069988 hasRelatedWork W2038162105 @default.
• W2019069988 hasRelatedWork W2081652198 @default.
• W2019069988 hasRelatedWork W2169021283 @default.
• W2019069988 hasRelatedWork W3088055158 @default.
• W2019069988 hasRelatedWork W3101395278 @default.
• W2019069988 hasRelatedWork W71898734 @default.
• W2019069988 hasVolume "2" @default.

• next