FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2896944650> ?p ?o ?g. }

• W2896944650 endingPage "58" @default.
• W2896944650 startingPage "58" @default.
• W2896944650 abstract "Subdwarf B stars are generally considered to be core helium-burning stars. However, most canonical sdB models have shown that they leave the sdB band (i.e., the region with 20,000 K ≤ Teff ≤ 40,000 K and ) after they have ignited helium in the shell. This means there will be a few shell helium-burning stars that have exhausted their helium in the core yet may still be located on the sdB band and should be considered as sdB stars too. But because they have effective temperature and gravity close to those of core helium-burning sdB stars, we cannot distinguish the two kinds of star just by atmospheric parameters. Some sdB stars display multimode pulsations. We thought that asteroseismology could offer some methods to distinguish the two kinds of sdB star. Core and shell helium-burning sdB stars have some obvious differences in structure and evolutionary track, which results in some clear differences in their pulsation properties. So, we may distinguish them by their pulsation properties such as the rates of change of period of the p-mode sdB pulsators, the numbers of mixed modes, and the period spacings of the g-mode sdB pulsators. We suggest that there are two special sdB stars (V391 Pegasi and PG 1605+072) that are likely shell helium-burning sdB stars." @default.
• W2896944650 created "2018-10-26" @default.
• W2896944650 creator A5005652582 @default.
• W2896944650 date "2018-10-11" @default.
• W2896944650 modified "2023-10-12" @default.
• W2896944650 title "Distinguishing Core and Shell Helium-burning Subdwarf B Stars by Asteroseismology" @default.
• W2896944650 cites W1965337953 @default.
• W2896944650 cites W1980672756 @default.
• W2896944650 cites W1982683895 @default.
• W2896944650 cites W1985702090 @default.
• W2896944650 cites W2006124034 @default.
• W2896944650 cites W2008663952 @default.
• W2896944650 cites W2009526636 @default.
• W2896944650 cites W2016488559 @default.
• W2896944650 cites W2022840985 @default.
• W2896944650 cites W2031705950 @default.
• W2896944650 cites W2032318068 @default.
• W2896944650 cites W2061637970 @default.
• W2896944650 cites W2062177733 @default.
• W2896944650 cites W2073306151 @default.
• W2896944650 cites W2074290792 @default.
• W2896944650 cites W2080866722 @default.
• W2896944650 cites W2090645204 @default.
• W2896944650 cites W2098427694 @default.
• W2896944650 cites W2103834171 @default.
• W2896944650 cites W2108910145 @default.
• W2896944650 cites W2136569281 @default.
• W2896944650 cites W2153663667 @default.
• W2896944650 cites W2155160488 @default.
• W2896944650 cites W2156831129 @default.
• W2896944650 cites W2167434382 @default.
• W2896944650 cites W2536938336 @default.
• W2896944650 cites W2548468810 @default.
• W2896944650 cites W2579898246 @default.
• W2896944650 cites W2904096024 @default.
• W2896944650 cites W3009883955 @default.
• W2896944650 cites W3097976388 @default.
• W2896944650 cites W3098350701 @default.
• W2896944650 cites W3099006993 @default.
• W2896944650 cites W3100270481 @default.
• W2896944650 cites W3102272565 @default.
• W2896944650 cites W3102529761 @default.
• W2896944650 cites W3103198216 @default.
• W2896944650 cites W3103590648 @default.
• W2896944650 cites W3103999057 @default.
• W2896944650 cites W3122852077 @default.
• W2896944650 cites W3123841297 @default.
• W2896944650 doi "https://doi.org/10.3847/1538-4357/aadd05" @default.
• W2896944650 hasPublicationYear "2018" @default.
• W2896944650 type Work @default.
• W2896944650 sameAs 2896944650 @default.
• W2896944650 citedByCount "2" @default.
• W2896944650 countsByYear W28969446502022 @default.
• W2896944650 countsByYear W28969446502023 @default.
• W2896944650 crossrefType "journal-article" @default.
• W2896944650 hasAuthorship W2896944650A5005652582 @default.
• W2896944650 hasBestOaLocation W28969446501 @default.
• W2896944650 hasConcept C110896241 @default.
• W2896944650 hasConcept C121332964 @default.
• W2896944650 hasConcept C1276947 @default.
• W2896944650 hasConcept C150846664 @default.
• W2896944650 hasConcept C164546044 @default.
• W2896944650 hasConcept C17352008 @default.
• W2896944650 hasConcept C178075534 @default.
• W2896944650 hasConcept C184779094 @default.
• W2896944650 hasConcept C197445014 @default.
• W2896944650 hasConcept C44870925 @default.
• W2896944650 hasConcept C54002840 @default.
• W2896944650 hasConcept C546029482 @default.
• W2896944650 hasConcept C67258758 @default.
• W2896944650 hasConcept C80518518 @default.
• W2896944650 hasConcept C99465377 @default.
• W2896944650 hasConceptScore W2896944650C110896241 @default.
• W2896944650 hasConceptScore W2896944650C121332964 @default.
• W2896944650 hasConceptScore W2896944650C1276947 @default.
• W2896944650 hasConceptScore W2896944650C150846664 @default.
• W2896944650 hasConceptScore W2896944650C164546044 @default.
• W2896944650 hasConceptScore W2896944650C17352008 @default.
• W2896944650 hasConceptScore W2896944650C178075534 @default.
• W2896944650 hasConceptScore W2896944650C184779094 @default.
• W2896944650 hasConceptScore W2896944650C197445014 @default.
• W2896944650 hasConceptScore W2896944650C44870925 @default.
• W2896944650 hasConceptScore W2896944650C54002840 @default.
• W2896944650 hasConceptScore W2896944650C546029482 @default.
• W2896944650 hasConceptScore W2896944650C67258758 @default.
• W2896944650 hasConceptScore W2896944650C80518518 @default.
• W2896944650 hasConceptScore W2896944650C99465377 @default.
• W2896944650 hasIssue "1" @default.
• W2896944650 hasLocation W28969446501 @default.
• W2896944650 hasOpenAccess W2896944650 @default.
• W2896944650 hasPrimaryLocation W28969446501 @default.
• W2896944650 hasRelatedWork W1627037870 @default.
• W2896944650 hasRelatedWork W1676627156 @default.
• W2896944650 hasRelatedWork W1677115070 @default.
• W2896944650 hasRelatedWork W1986400869 @default.
• W2896944650 hasRelatedWork W1992807432 @default.
• W2896944650 hasRelatedWork W2108450312 @default.
• W2896944650 hasRelatedWork W2147133951 @default.

• next