FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W1990141485> ?p ?o ?g. }

• W1990141485 endingPage "L78" @default.
• W1990141485 startingPage "L75" @default.
• W1990141485 abstract "The total ultraviolet (UV) flux (from 1412 to 2718 A) of M101 is compared on a pixel-to-pixel basis with the total far-infrared (FIR) flux (from 60 to 170 μm) using the maps of the galaxy taken by the Galaxy Evolution Explorer (GALEX) in the near-UV and far-UV and by the Infrared Space Observatory (ISO) at 60, 100, and 170 μm. The main result of this investigation is the discovery of a tight dependence of the FIR/UV ratio on radius, with values monotonically decreasing from ~4 in the nuclear region to nearly zero toward the edge of the optical disk. Although the tightness of this dependence is in part attributable to resolution effects, the result is consistent with the presence of a large-scale distribution of diffuse dust having a face-on optical depth that decreases with radius and that dominates over the more localized variations in opacity between the arm and interarm regions. We also find a trend for the FIR/UV ratio of taking on higher values in the regions of diffuse interarm emission than in the spiral-arm regions, at a given radius. This is interpreted quantitatively in terms of the escape probability of UV photons from spiral arms and their subsequent scattering in the interarm regions, and in terms of the larger relative contribution of optical photons to the heating of the dust in the interarm regions." @default.
• W1990141485 created "2016-06-24" @default.
• W1990141485 creator A5006293834 @default.
• W1990141485 creator A5011812052 @default.
• W1990141485 creator A5017671909 @default.
• W1990141485 creator A5019891335 @default.
• W1990141485 creator A5019995204 @default.
• W1990141485 creator A5023108247 @default.
• W1990141485 creator A5024725545 @default.
• W1990141485 creator A5028301941 @default.
• W1990141485 creator A5029381523 @default.
• W1990141485 creator A5032893133 @default.
• W1990141485 creator A5035116183 @default.
• W1990141485 creator A5035238229 @default.
• W1990141485 creator A5036805589 @default.
• W1990141485 creator A5037270981 @default.
• W1990141485 creator A5042509911 @default.
• W1990141485 creator A5046185531 @default.
• W1990141485 creator A5051909754 @default.
• W1990141485 creator A5055504752 @default.
• W1990141485 creator A5062572322 @default.
• W1990141485 creator A5075591111 @default.
• W1990141485 creator A5076173407 @default.
• W1990141485 creator A5077544810 @default.
• W1990141485 creator A5079787542 @default.
• W1990141485 creator A5080198665 @default.
• W1990141485 creator A5085997799 @default.
• W1990141485 creator A5091055123 @default.
• W1990141485 date "2005-01-17" @default.
• W1990141485 modified "2023-10-05" @default.
• W1990141485 title "A Comparative Study of the Spatial Distribution of Ultraviolet and Far-Infrared Fluxes from M101" @default.
• W1990141485 cites W1975826789 @default.
• W1990141485 cites W1981389634 @default.
• W1990141485 cites W1986549462 @default.
• W1990141485 cites W1996537612 @default.
• W1990141485 cites W1997377098 @default.
• W1990141485 cites W1999182952 @default.
• W1990141485 cites W2007993160 @default.
• W1990141485 cites W2009126121 @default.
• W1990141485 cites W2015733060 @default.
• W1990141485 cites W2046523578 @default.
• W1990141485 cites W2052179733 @default.
• W1990141485 cites W2055889513 @default.
• W1990141485 cites W2074056485 @default.
• W1990141485 cites W2085797005 @default.
• W1990141485 cites W2095125567 @default.
• W1990141485 cites W3099369643 @default.
• W1990141485 cites W3101200639 @default.
• W1990141485 cites W3103059900 @default.
• W1990141485 cites W3103530000 @default.
• W1990141485 cites W4296153596 @default.
• W1990141485 cites W4298872669 @default.
• W1990141485 doi "https://doi.org/10.1086/422991" @default.
• W1990141485 hasPublicationYear "2005" @default.
• W1990141485 type Work @default.
• W1990141485 sameAs 1990141485 @default.
• W1990141485 citedByCount "43" @default.
• W1990141485 countsByYear W19901414852012 @default.
• W1990141485 countsByYear W19901414852013 @default.
• W1990141485 countsByYear W19901414852015 @default.
• W1990141485 countsByYear W19901414852018 @default.
• W1990141485 crossrefType "journal-article" @default.
• W1990141485 hasAuthorship W1990141485A5006293834 @default.
• W1990141485 hasAuthorship W1990141485A5011812052 @default.
• W1990141485 hasAuthorship W1990141485A5017671909 @default.
• W1990141485 hasAuthorship W1990141485A5019891335 @default.
• W1990141485 hasAuthorship W1990141485A5019995204 @default.
• W1990141485 hasAuthorship W1990141485A5023108247 @default.
• W1990141485 hasAuthorship W1990141485A5024725545 @default.
• W1990141485 hasAuthorship W1990141485A5028301941 @default.
• W1990141485 hasAuthorship W1990141485A5029381523 @default.
• W1990141485 hasAuthorship W1990141485A5032893133 @default.
• W1990141485 hasAuthorship W1990141485A5035116183 @default.
• W1990141485 hasAuthorship W1990141485A5035238229 @default.
• W1990141485 hasAuthorship W1990141485A5036805589 @default.
• W1990141485 hasAuthorship W1990141485A5037270981 @default.
• W1990141485 hasAuthorship W1990141485A5042509911 @default.
• W1990141485 hasAuthorship W1990141485A5046185531 @default.
• W1990141485 hasAuthorship W1990141485A5051909754 @default.
• W1990141485 hasAuthorship W1990141485A5055504752 @default.
• W1990141485 hasAuthorship W1990141485A5062572322 @default.
• W1990141485 hasAuthorship W1990141485A5075591111 @default.
• W1990141485 hasAuthorship W1990141485A5076173407 @default.
• W1990141485 hasAuthorship W1990141485A5077544810 @default.
• W1990141485 hasAuthorship W1990141485A5079787542 @default.
• W1990141485 hasAuthorship W1990141485A5080198665 @default.
• W1990141485 hasAuthorship W1990141485A5085997799 @default.
• W1990141485 hasAuthorship W1990141485A5091055123 @default.
• W1990141485 hasBestOaLocation W19901414851 @default.
• W1990141485 hasConcept C120665830 @default.
• W1990141485 hasConcept C121332964 @default.
• W1990141485 hasConcept C127313418 @default.
• W1990141485 hasConcept C1276947 @default.
• W1990141485 hasConcept C131432281 @default.
• W1990141485 hasConcept C150846664 @default.
• W1990141485 hasConcept C158355884 @default.
• W1990141485 hasConcept C2776798109 @default.
• W1990141485 hasConcept C2777016058 @default.

• next