Modelling the Nonthermal Emission of the Pulsar Wind Nebula MSH 15-52
Author : Sebastian Meßlinger
Publisher :
Page : 34 pages
File Size : 10,42 MB
Release : 2013
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Author : Sebastian Meßlinger
Publisher :
Page : 34 pages
File Size : 10,42 MB
Release : 2013
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Author : Philipp Willmann
Publisher :
Page : 50 pages
File Size : 13,47 MB
Release : 2012
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Author : Diego F. Torres
Publisher : Springer
Page : 318 pages
File Size : 45,54 MB
Release : 2017-11-13
Category : Science
ISBN : 3319630318
In 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.
Author : Markus Holler
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Page : 60 pages
File Size : 42,54 MB
Release : 2010
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Author : Nanda Rea
Publisher : Springer Science & Business Media
Page : 656 pages
File Size : 28,65 MB
Release : 2011-02-04
Category : Science
ISBN : 3642172512
The aim of the inaugural meeting of the Sant Cugat Forum on Astrophysics was to address, in a global context, the current understanding of and challenges in high-energy emissions from isolated and non-isolated neutron stars, and to confront the theoretical picture with observations of both the Fermi satellite and the currently operating ground-based Cherenkov telescopes. Participants have also discussed the prospects for possible observations with planned instruments across the multi-wavelength spectrum (e.g. SKA, LOFAR, E-VLT, IXO, CTA) and how they will impact our theoretical understanding of these systems. In keeping with the goals of the Forum, this book not only represents the proceedings of the meeting, but also a reflection on the state-of-the-art in the topic.
Author : 梁偉恩
Publisher :
Page : 212 pages
File Size : 10,57 MB
Release : 2018
Category : Pulsars
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Author : Barbara Olmi
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Page : pages
File Size : 45,99 MB
Release : 2015
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Author : Fabian Matthias Schöck
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Page : 155 pages
File Size : 18,70 MB
Release : 2010
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Author : Christoph Bürkel
Publisher :
Page : 33 pages
File Size : 26,23 MB
Release : 2012
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Page : pages
File Size : 25,88 MB
Release : 2015
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I analyze filament G359.97-0.038 by incorporating broad-band morphological and spectral data from radio (5.5 and 8.3 GHz) and X-ray data with NuSTAR data. I conclude that it is not a PWN but more likely the result of an interaction between the Sgr A East remnant and the nearby molecular cloud. Lastly I observe the filament G0.13-0.11, likely a PWN elongated by the ram pressure from the nearby Radio Arc.