Matches in SemOpenAlex for { <https://semopenalex.org/work/W2044103620> ?p ?o ?g. }
- W2044103620 endingPage "17" @default.
- W2044103620 startingPage "12" @default.
- W2044103620 abstract "Pulsar wind nebulae are a prominent class of very high energy (E > 0.1 TeV) Galactic sources. Their Gamma-ray spectra are interpreted as due to inverse Compton scattering of ultrarelativistic electrons on the ambient photons, whereas the X-ray spectra are due to synchrotron emission. We investigate the relation between the Gamma- and-X-ray emission and the pulsars' spin-down luminosity and characteristic age. We find that the distance-independent Gamma- to X-ray flux ratio of the nebulae is inversely proportional to the spin-down luminosity, (propto dot{E}^-1.9), while it appears proportional to the characteristic age, (propto tau_c^2.2), of the parent pulsar. We interpret these results as due to the evolution of the electron energy distribution and the nebular dynamics, supporting the idea of so-called relic pulsar wind nebulae. These empirical relations provide a new tool to classify unidentified diffuse Gamma-ray sources and to estimate the spin-down luminosity and characteristic age of rotation powered pulsars with no detected pulsation from the X- and Gamma-ray properties of the associated pulsar wind nebulae. We apply these relations to predict the spin-down luminosity and characteristic age of four (so far unpulsing) candidate pulsars associated to wind nebulae." @default.
- W2044103620 created "2016-06-24" @default.
- W2044103620 creator A5000697015 @default.
- W2044103620 creator A5014980340 @default.
- W2044103620 creator A5016341295 @default.
- W2044103620 creator A5018954883 @default.
- W2044103620 creator A5020987575 @default.
- W2044103620 creator A5053059499 @default.
- W2044103620 creator A5056350999 @default.
- W2044103620 creator A5060846079 @default.
- W2044103620 creator A5065755325 @default.
- W2044103620 creator A5084086175 @default.
- W2044103620 date "2009-03-14" @default.
- W2044103620 modified "2023-09-30" @default.
- W2044103620 title "THE EVOLUTION OF THE γ- AND X-RAY LUMINOSITIES OF PULSAR WIND NEBULAE" @default.
- W2044103620 cites W1679241061 @default.
- W2044103620 cites W1973820399 @default.
- W2044103620 cites W1980396493 @default.
- W2044103620 cites W1985169389 @default.
- W2044103620 cites W1990640604 @default.
- W2044103620 cites W1992768712 @default.
- W2044103620 cites W2000917280 @default.
- W2044103620 cites W2008405546 @default.
- W2044103620 cites W2027148204 @default.
- W2044103620 cites W2027164753 @default.
- W2044103620 cites W2031246503 @default.
- W2044103620 cites W2032322105 @default.
- W2044103620 cites W2034065304 @default.
- W2044103620 cites W2036416640 @default.
- W2044103620 cites W2039003267 @default.
- W2044103620 cites W2043272552 @default.
- W2044103620 cites W2047988398 @default.
- W2044103620 cites W2054923548 @default.
- W2044103620 cites W2060626812 @default.
- W2044103620 cites W2066358160 @default.
- W2044103620 cites W2067874678 @default.
- W2044103620 cites W2068326417 @default.
- W2044103620 cites W2072831010 @default.
- W2044103620 cites W2088832460 @default.
- W2044103620 cites W2090668718 @default.
- W2044103620 cites W2090726830 @default.
- W2044103620 cites W2104721808 @default.
- W2044103620 cites W2121927671 @default.
- W2044103620 cites W2122737259 @default.
- W2044103620 cites W2123039622 @default.
- W2044103620 cites W2124619345 @default.
- W2044103620 cites W2135621672 @default.
- W2044103620 cites W2140566529 @default.
- W2044103620 cites W2149330123 @default.
- W2044103620 cites W2161172896 @default.
- W2044103620 cites W2163021058 @default.
- W2044103620 cites W2163770281 @default.
- W2044103620 cites W2167296890 @default.
- W2044103620 cites W2952070202 @default.
- W2044103620 cites W3098231965 @default.
- W2044103620 cites W3098729955 @default.
- W2044103620 cites W3099320285 @default.
- W2044103620 cites W3099369026 @default.
- W2044103620 cites W3100265633 @default.
- W2044103620 cites W3101499996 @default.
- W2044103620 cites W3103335596 @default.
- W2044103620 cites W3103598994 @default.
- W2044103620 cites W3104308207 @default.
- W2044103620 cites W3104395252 @default.
- W2044103620 cites W3125814380 @default.
- W2044103620 doi "https://doi.org/10.1088/0004-637x/694/1/12" @default.
- W2044103620 hasPublicationYear "2009" @default.
- W2044103620 type Work @default.
- W2044103620 sameAs 2044103620 @default.
- W2044103620 citedByCount "87" @default.
- W2044103620 countsByYear W20441036202012 @default.
- W2044103620 countsByYear W20441036202013 @default.
- W2044103620 countsByYear W20441036202014 @default.
- W2044103620 countsByYear W20441036202015 @default.
- W2044103620 countsByYear W20441036202016 @default.
- W2044103620 countsByYear W20441036202017 @default.
- W2044103620 countsByYear W20441036202018 @default.
- W2044103620 countsByYear W20441036202019 @default.
- W2044103620 countsByYear W20441036202020 @default.
- W2044103620 countsByYear W20441036202021 @default.
- W2044103620 countsByYear W20441036202022 @default.
- W2044103620 countsByYear W20441036202023 @default.
- W2044103620 crossrefType "journal-article" @default.
- W2044103620 hasAuthorship W2044103620A5000697015 @default.
- W2044103620 hasAuthorship W2044103620A5014980340 @default.
- W2044103620 hasAuthorship W2044103620A5016341295 @default.
- W2044103620 hasAuthorship W2044103620A5018954883 @default.
- W2044103620 hasAuthorship W2044103620A5020987575 @default.
- W2044103620 hasAuthorship W2044103620A5053059499 @default.
- W2044103620 hasAuthorship W2044103620A5056350999 @default.
- W2044103620 hasAuthorship W2044103620A5060846079 @default.
- W2044103620 hasAuthorship W2044103620A5065755325 @default.
- W2044103620 hasAuthorship W2044103620A5084086175 @default.
- W2044103620 hasBestOaLocation W20441036201 @default.
- W2044103620 hasConcept C110363677 @default.
- W2044103620 hasConcept C121332964 @default.
- W2044103620 hasConcept C12287442 @default.
- W2044103620 hasConcept C1276947 @default.