FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2030359568> ?p ?o ?g. }

• W2030359568 endingPage "1386" @default.
• W2030359568 startingPage "1378" @default.
• W2030359568 abstract "We study the evolution of gas in H ii regions around the first stars after the exciting stars end their lives. If the first star in a small halo dies without supernova (SN), subsequent star formation is possible in the same halo. We thus investigate the effect of ionization on subsequent star formation within small haloes in the early Universe using one-dimensional hydrodynamics with spherical symmetry along with non-equilibrium primordial gas chemistry. We find that the enhanced electron fraction facilitates the formation of molecular hydrogen at the cores of these haloes. The low temperature circumstances produced by the H2 cooling is favourable to HD formation and the resultant cooling further drops the temperature below 100 K. Consequently, low-mass stars with primordial abundances can form even in a small halo. After accreting the interstellar metals, these stars might resemble low-mass ultra metal-poor stars discovered in the present-day Galactic halo." @default.
• W2030359568 created "2016-06-24" @default.
• W2030359568 creator A5066500271 @default.
• W2030359568 creator A5090162014 @default.
• W2030359568 date "2005-12-01" @default.
• W2030359568 modified "2023-10-15" @default.
• W2030359568 title "Formation of Population III stars in fossil H ii regions: significance of HD" @default.
• W2030359568 cites W1970129433 @default.
• W2030359568 cites W1971356221 @default.
• W2030359568 cites W1975314963 @default.
• W2030359568 cites W1978253505 @default.
• W2030359568 cites W1983471014 @default.
• W2030359568 cites W1988090704 @default.
• W2030359568 cites W2007687569 @default.
• W2030359568 cites W2013997547 @default.
• W2030359568 cites W2019428480 @default.
• W2030359568 cites W2019771205 @default.
• W2030359568 cites W2022782755 @default.
• W2030359568 cites W2029047760 @default.
• W2030359568 cites W2029799079 @default.
• W2030359568 cites W2035382618 @default.
• W2030359568 cites W2036179433 @default.
• W2030359568 cites W2040912209 @default.
• W2030359568 cites W2044643318 @default.
• W2030359568 cites W2045229244 @default.
• W2030359568 cites W2061378179 @default.
• W2030359568 cites W2065198265 @default.
• W2030359568 cites W2067827212 @default.
• W2030359568 cites W2077678988 @default.
• W2030359568 cites W2079349557 @default.
• W2030359568 cites W2096369604 @default.
• W2030359568 cites W2097043658 @default.
• W2030359568 cites W2102964970 @default.
• W2030359568 cites W2118265220 @default.
• W2030359568 cites W2121335788 @default.
• W2030359568 cites W2129495060 @default.
• W2030359568 cites W2951034677 @default.
• W2030359568 cites W3098202963 @default.
• W2030359568 cites W3098579036 @default.
• W2030359568 cites W3100110286 @default.
• W2030359568 cites W3100685835 @default.
• W2030359568 cites W3106012295 @default.
• W2030359568 cites W3106194983 @default.
• W2030359568 cites W3106353668 @default.
• W2030359568 doi "https://doi.org/10.1111/j.1365-2966.2005.09685.x" @default.
• W2030359568 hasPublicationYear "2005" @default.
• W2030359568 type Work @default.
• W2030359568 sameAs 2030359568 @default.
• W2030359568 citedByCount "66" @default.
• W2030359568 countsByYear W20303595682012 @default.
• W2030359568 countsByYear W20303595682013 @default.
• W2030359568 countsByYear W20303595682014 @default.
• W2030359568 countsByYear W20303595682015 @default.
• W2030359568 countsByYear W20303595682016 @default.
• W2030359568 countsByYear W20303595682018 @default.
• W2030359568 countsByYear W20303595682019 @default.
• W2030359568 countsByYear W20303595682020 @default.
• W2030359568 countsByYear W20303595682022 @default.
• W2030359568 countsByYear W20303595682023 @default.
• W2030359568 crossrefType "journal-article" @default.
• W2030359568 hasAuthorship W2030359568A5066500271 @default.
• W2030359568 hasAuthorship W2030359568A5090162014 @default.
• W2030359568 hasBestOaLocation W20303595681 @default.
• W2030359568 hasConcept C121332964 @default.
• W2030359568 hasConcept C125857072 @default.
• W2030359568 hasConcept C127592171 @default.
• W2030359568 hasConcept C1276947 @default.
• W2030359568 hasConcept C144024400 @default.
• W2030359568 hasConcept C149923435 @default.
• W2030359568 hasConcept C150846664 @default.
• W2030359568 hasConcept C184665706 @default.
• W2030359568 hasConcept C2908647359 @default.
• W2030359568 hasConcept C44870925 @default.
• W2030359568 hasConcept C48387981 @default.
• W2030359568 hasConcept C98444146 @default.
• W2030359568 hasConceptScore W2030359568C121332964 @default.
• W2030359568 hasConceptScore W2030359568C125857072 @default.
• W2030359568 hasConceptScore W2030359568C127592171 @default.
• W2030359568 hasConceptScore W2030359568C1276947 @default.
• W2030359568 hasConceptScore W2030359568C144024400 @default.
• W2030359568 hasConceptScore W2030359568C149923435 @default.
• W2030359568 hasConceptScore W2030359568C150846664 @default.
• W2030359568 hasConceptScore W2030359568C184665706 @default.
• W2030359568 hasConceptScore W2030359568C2908647359 @default.
• W2030359568 hasConceptScore W2030359568C44870925 @default.
• W2030359568 hasConceptScore W2030359568C48387981 @default.
• W2030359568 hasConceptScore W2030359568C98444146 @default.
• W2030359568 hasIssue "4" @default.
• W2030359568 hasLocation W20303595681 @default.
• W2030359568 hasLocation W20303595682 @default.
• W2030359568 hasLocation W20303595683 @default.
• W2030359568 hasOpenAccess W2030359568 @default.
• W2030359568 hasPrimaryLocation W20303595681 @default.
• W2030359568 hasRelatedWork W1578211655 @default.
• W2030359568 hasRelatedWork W1858127741 @default.
• W2030359568 hasRelatedWork W1999895351 @default.
• W2030359568 hasRelatedWork W2039390883 @default.
• W2030359568 hasRelatedWork W2886224880 @default.

• next