FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2089149194> ?p ?o ?g. }

• W2089149194 endingPage "1316" @default.
• W2089149194 startingPage "1307" @default.
• W2089149194 abstract "If Type II supernovae – the evolutionary end points of short-lived, massive stars – produce a significant quantity of dust (>0.1 M⊙) then they can explain the rest-frame far-infrared emission seen in galaxies and quasars in the first Gyr of the Universe. Submillimetre (submm) observations of the Galactic supernova remnant, Cas A, provided the first observational evidence for the formation of significant quantities of dust in Type II supernovae. In this paper, we present new data which show that the submm emission from Cas A is polarized at a level significantly higher than that of its synchrotron emission. The orientation is consistent with that of the magnetic field in Cas A, implying that the polarized submm emission is associated with the remnant. No known mechanism would vary the synchrotron polarization in this way and so we attribute the excess polarized submm flux to cold dust within the remnant, providing fresh evidence that cosmic dust can form rapidly. This is supported by the presence of both polarized and unpolarized dust emission in the north of the remnant where there is no contamination from foreground molecular clouds. The inferred dust polarization fraction is unprecedented (fpol∼ 30 per cent) which, coupled with the brief time-scale available for grain alignment (<300 yr), suggests that supernova dust differs from that seen in other Galactic sources (where fpol= 2−7 per cent) or that a highly efficient grain alignment process must operate in the environment of a supernova remnant." @default.
• W2089149194 created "2016-06-24" @default.
• W2089149194 creator A5000047338 @default.
• W2089149194 creator A5014375153 @default.
• W2089149194 creator A5027826119 @default.
• W2089149194 creator A5046254773 @default.
• W2089149194 creator A5053593436 @default.
• W2089149194 creator A5060096577 @default.
• W2089149194 creator A5062504729 @default.
• W2089149194 creator A5069833094 @default.
• W2089149194 creator A5071124103 @default.
• W2089149194 creator A5079763409 @default.
• W2089149194 date "2009-04-11" @default.
• W2089149194 modified "2023-09-26" @default.
• W2089149194 title "Cassiopeia A: dust factory revealed via submillimetre polarimetry" @default.
• W2089149194 cites W1485133653 @default.
• W2089149194 cites W1963485929 @default.
• W2089149194 cites W1966858780 @default.
• W2089149194 cites W1968718345 @default.
• W2089149194 cites W1973443151 @default.
• W2089149194 cites W1973954037 @default.
• W2089149194 cites W1977390196 @default.
• W2089149194 cites W1978468051 @default.
• W2089149194 cites W1980124829 @default.
• W2089149194 cites W1983032649 @default.
• W2089149194 cites W1986648137 @default.
• W2089149194 cites W1999903618 @default.
• W2089149194 cites W2001530733 @default.
• W2089149194 cites W2003102625 @default.
• W2089149194 cites W2003688880 @default.
• W2089149194 cites W2013064166 @default.
• W2089149194 cites W2020343420 @default.
• W2089149194 cites W2026560309 @default.
• W2089149194 cites W2031615933 @default.
• W2089149194 cites W2034557909 @default.
• W2089149194 cites W2035498751 @default.
• W2089149194 cites W2036864532 @default.
• W2089149194 cites W2042492191 @default.
• W2089149194 cites W2047615974 @default.
• W2089149194 cites W2051661622 @default.
• W2089149194 cites W2053402415 @default.
• W2089149194 cites W2056064821 @default.
• W2089149194 cites W2056400752 @default.
• W2089149194 cites W2062166036 @default.
• W2089149194 cites W2064554270 @default.
• W2089149194 cites W2067518128 @default.
• W2089149194 cites W2083516594 @default.
• W2089149194 cites W2093830760 @default.
• W2089149194 cites W2094079825 @default.
• W2089149194 cites W2108093615 @default.
• W2089149194 cites W2108445226 @default.
• W2089149194 cites W2109401568 @default.
• W2089149194 cites W2118686098 @default.
• W2089149194 cites W2134252664 @default.
• W2089149194 cites W2134675769 @default.
• W2089149194 cites W2145265132 @default.
• W2089149194 cites W2177455466 @default.
• W2089149194 cites W2951313103 @default.
• W2089149194 cites W3099885840 @default.
• W2089149194 cites W3100689270 @default.
• W2089149194 cites W3101016936 @default.
• W2089149194 cites W3102101987 @default.
• W2089149194 cites W3102724155 @default.
• W2089149194 cites W3104080068 @default.
• W2089149194 cites W3104459078 @default.
• W2089149194 cites W3105101348 @default.
• W2089149194 cites W3105221658 @default.
• W2089149194 cites W3105887755 @default.
• W2089149194 cites W3106494760 @default.
• W2089149194 doi "https://doi.org/10.1111/j.1365-2966.2009.14453.x" @default.
• W2089149194 hasPublicationYear "2009" @default.
• W2089149194 type Work @default.
• W2089149194 sameAs 2089149194 @default.
• W2089149194 citedByCount "88" @default.
• W2089149194 countsByYear W20891491942012 @default.
• W2089149194 countsByYear W20891491942013 @default.
• W2089149194 countsByYear W20891491942014 @default.
• W2089149194 countsByYear W20891491942015 @default.
• W2089149194 countsByYear W20891491942016 @default.
• W2089149194 countsByYear W20891491942017 @default.
• W2089149194 countsByYear W20891491942018 @default.
• W2089149194 countsByYear W20891491942019 @default.
• W2089149194 countsByYear W20891491942020 @default.
• W2089149194 countsByYear W20891491942021 @default.
• W2089149194 countsByYear W20891491942022 @default.
• W2089149194 countsByYear W20891491942023 @default.
• W2089149194 crossrefType "journal-article" @default.
• W2089149194 hasAuthorship W2089149194A5000047338 @default.
• W2089149194 hasAuthorship W2089149194A5014375153 @default.
• W2089149194 hasAuthorship W2089149194A5027826119 @default.
• W2089149194 hasAuthorship W2089149194A5046254773 @default.
• W2089149194 hasAuthorship W2089149194A5053593436 @default.
• W2089149194 hasAuthorship W2089149194A5060096577 @default.
• W2089149194 hasAuthorship W2089149194A5062504729 @default.
• W2089149194 hasAuthorship W2089149194A5069833094 @default.
• W2089149194 hasAuthorship W2089149194A5071124103 @default.
• W2089149194 hasAuthorship W2089149194A5079763409 @default.
• W2089149194 hasBestOaLocation W20891491941 @default.

• next