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001 | u375892 | ||
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005 | 20160812084346.0 | ||
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008 | 110714s2011 gw | s |||| 0|eng d | ||
020 |
_a9783642196270 _9978-3-642-19627-0 |
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040 | _cMX-MeUAM | ||
050 | 4 | _aQB1-991 | |
050 | 4 | _aQB460-466 | |
050 | 4 | _aQB980-991 | |
082 | 0 | 4 |
_a520 _223 |
100 | 1 |
_aKeane, Evan Francis. _eauthor. |
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245 | 1 | 4 |
_aThe Transient Radio Sky _h[recurso electrónico] / _cby Evan Francis Keane. |
264 | 1 |
_aBerlin, Heidelberg : _bSpringer Berlin Heidelberg : _bImprint: Springer, _c2011. |
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300 |
_aXIV, 190 p. _bonline resource. |
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336 |
_atext _btxt _2rdacontent |
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_acomputer _bc _2rdamedia |
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_aonline resource _bcr _2rdacarrier |
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_atext file _bPDF _2rda |
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490 | 1 |
_aSpringer Theses, _x2190-5053 |
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505 | 0 | _aTransients -- 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.-. | |
520 | _aThe 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. | ||
650 | 0 | _aPhysics. | |
650 | 0 | _aAstronomy. | |
650 | 1 | 4 | _aPhysics. |
650 | 2 | 4 | _aAstronomy, Astrophysics and Cosmology. |
650 | 2 | 4 | _aSpectroscopy and Microscopy. |
710 | 2 | _aSpringerLink (Online service) | |
773 | 0 | _tSpringer eBooks | |
776 | 0 | 8 |
_iPrinted edition: _z9783642196263 |
830 | 0 |
_aSpringer Theses, _x2190-5053 |
|
856 | 4 | 0 |
_zLibro electrónico _uhttp://148.231.10.114:2048/login?url=http://link.springer.com/book/10.1007/978-3-642-19627-0 |
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942 | _cLIBRO_ELEC | ||
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_c203772 _d203772 |