FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W4386114575> ?p ?o ?g. }

• W4386114575 endingPage "53" @default.
• W4386114575 startingPage "53" @default.
• W4386114575 abstract "Abstract We propose and apply a method to quantify the morphology of the large-scale ordered magnetic fields ( B -fields) in galaxies. This method is adapted from the analysis of Event Horizon Telescope polarization data. We compute a linear decomposition of the azimuthal modes of the polarization field in radial galactocentric bins. We apply this approach to five low-inclination spiral galaxies with both far-infrared (FIR: 154 μ m) dust polarimetric observations taken from the Survey of Extragalactic Magnetism with SOFIA (SALSA) and radio (6 cm) synchrotron polarization observations. We find that the main contribution to the B -field structure of these spiral galaxies comes from the m = 2 and m = 0 modes at FIR wavelengths and the m = 2 mode at radio wavelengths. The m = 2 mode has a spiral structure and is directly related to the magnetic pitch angle, while m = 0 has a constant B -field orientation. The FIR data tend to have a higher relative contribution from other modes than the radio data. The extreme case is NGC 6946: all modes contribute similarly in the FIR, while m = 2 still dominates in the radio. The average magnetic pitch angle in the FIR data is smaller and has greater angular dispersion than in the radio, indicating that the B -fields in the disk midplane traced by FIR dust polarization are more tightly wound and more chaotic than the B -field structure in the radio, which probes a larger volume. We argue that our approach is more flexible and model independent than standard techniques, while still producing consistent results where directly comparable." @default.
• W4386114575 created "2023-08-24" @default.
• W4386114575 creator A5005699219 @default.
• W4386114575 creator A5030061363 @default.
• W4386114575 creator A5065764349 @default.
• W4386114575 date "2023-08-22" @default.
• W4386114575 modified "2023-09-23" @default.
• W4386114575 title "The Structure of Magnetic Fields in Spiral Galaxies: A Radio and Far-infrared Polarimetric Analysis" @default.
• W4386114575 cites W1670650379 @default.
• W4386114575 cites W1848023164 @default.
• W4386114575 cites W1974973013 @default.
• W4386114575 cites W2011301426 @default.
• W4386114575 cites W2016888141 @default.
• W4386114575 cites W2017052513 @default.
• W4386114575 cites W2017627447 @default.
• W4386114575 cites W2041219985 @default.
• W4386114575 cites W2054899182 @default.
• W4386114575 cites W2057408271 @default.
• W4386114575 cites W2068939329 @default.
• W4386114575 cites W2071037908 @default.
• W4386114575 cites W2071900009 @default.
• W4386114575 cites W2074466769 @default.
• W4386114575 cites W2091021342 @default.
• W4386114575 cites W2099178377 @default.
• W4386114575 cites W2102017302 @default.
• W4386114575 cites W2117093954 @default.
• W4386114575 cites W2140662535 @default.
• W4386114575 cites W2145956230 @default.
• W4386114575 cites W2152127982 @default.
• W4386114575 cites W2165760757 @default.
• W4386114575 cites W2199495426 @default.
• W4386114575 cites W2884074461 @default.
• W4386114575 cites W2963150841 @default.
• W4386114575 cites W2995498358 @default.
• W4386114575 cites W3098227962 @default.
• W4386114575 cites W3099716850 @default.
• W4386114575 cites W3100655566 @default.
• W4386114575 cites W3101077302 @default.
• W4386114575 cites W3102488955 @default.
• W4386114575 cites W3103145119 @default.
• W4386114575 cites W3103271501 @default.
• W4386114575 cites W3105280731 @default.
• W4386114575 cites W3105566130 @default.
• W4386114575 cites W3106186675 @default.
• W4386114575 cites W3123001727 @default.
• W4386114575 cites W3137038733 @default.
• W4386114575 cites W3139022070 @default.
• W4386114575 cites W3150327101 @default.
• W4386114575 cites W3159522911 @default.
• W4386114575 cites W3200578993 @default.
• W4386114575 cites W3213197636 @default.
• W4386114575 cites W4292408406 @default.
• W4386114575 cites W4292923859 @default.
• W4386114575 cites W4293212596 @default.
• W4386114575 cites W4293802469 @default.
• W4386114575 cites W4294683734 @default.
• W4386114575 cites W4300445640 @default.
• W4386114575 cites W4313517956 @default.
• W4386114575 cites W4321503464 @default.
• W4386114575 cites W4362608962 @default.
• W4386114575 cites W4380047971 @default.
• W4386114575 cites W4384133715 @default.
• W4386114575 doi "https://doi.org/10.3847/1538-4357/ace4c0" @default.
• W4386114575 hasPublicationYear "2023" @default.
• W4386114575 type Work @default.
• W4386114575 citedByCount "0" @default.
• W4386114575 crossrefType "journal-article" @default.
• W4386114575 hasAuthorship W4386114575A5005699219 @default.
• W4386114575 hasAuthorship W4386114575A5030061363 @default.
• W4386114575 hasAuthorship W4386114575A5065764349 @default.
• W4386114575 hasBestOaLocation W43861145751 @default.
• W4386114575 hasConcept C107190969 @default.
• W4386114575 hasConcept C115260700 @default.
• W4386114575 hasConcept C120665830 @default.
• W4386114575 hasConcept C121332964 @default.
• W4386114575 hasConcept C1276947 @default.
• W4386114575 hasConcept C147789679 @default.
• W4386114575 hasConcept C185592680 @default.
• W4386114575 hasConcept C191486275 @default.
• W4386114575 hasConcept C20249676 @default.
• W4386114575 hasConcept C205049153 @default.
• W4386114575 hasConcept C28493345 @default.
• W4386114575 hasConcept C44870925 @default.
• W4386114575 hasConcept C520434653 @default.
• W4386114575 hasConcept C62520636 @default.
• W4386114575 hasConcept C63585750 @default.
• W4386114575 hasConcept C98444146 @default.
• W4386114575 hasConceptScore W4386114575C107190969 @default.
• W4386114575 hasConceptScore W4386114575C115260700 @default.
• W4386114575 hasConceptScore W4386114575C120665830 @default.
• W4386114575 hasConceptScore W4386114575C121332964 @default.
• W4386114575 hasConceptScore W4386114575C1276947 @default.
• W4386114575 hasConceptScore W4386114575C147789679 @default.
• W4386114575 hasConceptScore W4386114575C185592680 @default.
• W4386114575 hasConceptScore W4386114575C191486275 @default.
• W4386114575 hasConceptScore W4386114575C20249676 @default.
• W4386114575 hasConceptScore W4386114575C205049153 @default.
• W4386114575 hasConceptScore W4386114575C28493345 @default.

• next