The Transient Radio Sky

The high time-resolution radio sky represents unexplored astronomical territory. This thesis presents a study of the transient radio sky, focussing on millisecond scales. As such, the work is concerned primarily with neutron stars. In particular this research concentrates on a recently identified gr...

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Detalhes bibliográficos
Autor principal: Keane, Evan Francis
Formato: Livre numérique
Idioma:Anglais
Publicado em: Berlin, Heidelberg : Springer Berlin Heidelberg [20..].
Cham : Springer Nature
Edição:1st ed. 2011.
Colecção:Springer Theses, Recognizing Outstanding Ph.D. Research
Acesso em linha:Accès sur la plateforme de l'éditeur
Accès sur la plateforme Istex
Accès Université d'Orléans
Accès INSA CVL
Nota: Archives Springer e-books (Licence nationale)
Archives Springer e-books (Licence nationale)
Autres localisations: Voir dans le Sudoc
Edition sous un autre format:• The transient radio sky, doctoral thesis accepted by the University of Manchester, UK, Evan Francis Keane, 2011, Berlin, Springer, 1 vol. (XIII-190 p.), Springer theses, 3-642-19626-8
• The Transient Radio Sky, Texte imprimé, 9783642270543
• The transient radio sky, doctoral thesis accepted by the University of Manchester, UK, Evan Francis Keane, 2011, Berlin, Springer, 1 vol. (XIII-190 p.), Springer theses, 3-642-19626-8
• The Transient Radio Sky, Texte imprimé, 9783642196287
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505 1 |a Transients Neutron Stars NS Birthrates PMSingle RRAT Timing New Timing Solutions X-ray & Optical Observations RRATs: An Overview Conclusions Radio Astronomy Equations Neutron Stars: Supplementary Birthrates: Supplementary PMSingle: Supplementary.- 
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520 |a The high time-resolution radio sky represents unexplored astronomical territory. This thesis presents a study of the transient radio sky, focussing on millisecond scales. As such, the work is concerned primarily with neutron stars. In particular this research concentrates on a recently identified group of neutron stars, known as RRATs, which exhibit radio bursts every few minutes to every few hours. After analysing neutron star birthrates, a re-analysis of the Parkes Multibeam Pulsar Survey is described which has resulted in the discovery of 19 new transient radio sources. Of these, 12 have been seen to repeat and a followup campaign of observations has been undertaken. These studies have greatly increased our knowledge of the rotational properties of RRATs and enable us to conclude that they are pulsars with extreme nulling and/or pulse-to-pulse modulation. Although the evolution of neutron stars post-supernova is not yet understood, it seems that RRATs fit into the emerging picture in which pulsar magnetospheres switch between stable configurations 
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