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010   $a3-319-63031-8
024 7 $a10.1007/978-3-319-63031-1
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035   $a(DE-He213)978-3-319-63031-1
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035   $a(PPN)221251898
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100   $a20171114d2017      u|         0
101 0 $aeng
135   $aurnn|008mamaa
181   $ctxt$2rdacontent
182   $cc$2rdamedia
183   $acr$2rdacarrier
200 10$aModelling Pulsar Wind Nebulae /$fedited by Diego F. Torres
205   $a1st ed. 2017.
210  1$aCham :$cSpringer International Publishing :$cImprint: Springer,$d2017.
215   $a1 online resource (XI, 313 p. 121 illus., 105 illus. in color.) 
225 1 $aAstrophysics and Space Science Library,$x0067-0057 ;$v446
311   $a3-319-63030-X 
320   $aIncludes bibliographical references at the end of each chapters and index.
330   $aIn view of the current and forthcoming observational data on pulsar wind nebulae, this book offers an assessment of the theoretical state of the art of modelling them. The expert authors also review the observational status of the field and provide an outlook for future developments. During the last few years, significant progress on the study of pulsar wind nebulae (PWNe) has been attained both from a theoretical and an observational perspective, perhaps focusing on the closest, more energetic, and best studied nebula: the Crab, which appears in the cover. Now, the number of TeV detected PWNe is similar to the number of characterized nebulae observed at other frequencies over decades of observations. And in just a few years, the Cherenkov Telescope Array will increase this number to several hundreds, actually providing an essentially complete account of TeV emitting PWNe in the Galaxy. At the other end of the multi-frequency spectrum, the SKA and its pathfinder instruments, will reveal thousands of new pulsars, and map in exquisite detail the radiation surrounding them for several hundreds of nebulae. By carefully reviewing the state of the art in pulsar nebula research this book prepares scientists and PhD students for future work and progress in the field.
410  0$aAstrophysics and Space Science Library,$x0067-0057 ;$v446
606   $aAstrophysics
606   $aObservations, Astronomical
606   $aAstronomy?Observations
606   $aMathematical physics
606   $aAstrophysics and Astroparticles$3https://scigraph.springernature.com/ontologies/product-market-codes/P22022
606   $aAstronomy, Observations and Techniques$3https://scigraph.springernature.com/ontologies/product-market-codes/P22014
606   $aTheoretical, Mathematical and Computational Physics$3https://scigraph.springernature.com/ontologies/product-market-codes/P19005
615  0$aAstrophysics.
615  0$aObservations, Astronomical.
615  0$aAstronomy?Observations.
615  0$aMathematical physics.
615 14$aAstrophysics and Astroparticles.
615 24$aAstronomy, Observations and Techniques.
615 24$aTheoretical, Mathematical and Computational Physics.
676   $a523.1135
702   $aTorres$b Diego F$4edt$4http://id.loc.gov/vocabulary/relators/edt
801  0$bMiAaPQ
801  1$bMiAaPQ
801  2$bMiAaPQ
906   $aBOOK
912   $a9910254587703321
996   $aModelling Pulsar Wind Nebulae$91832391
997   $aUNINA