000			04426nam a22003735i 4500
001			298293
003			MX-SnUAN
005			20160429155457.0
007			cr nn 008mamaa
008			150903s2009 gw | o |||| 0|eng d
020			_a9783540769651 _99783540769651
024	7		_a10.1007/9783540769651 _2doi
035			_avtls000351323
039		9	_a201509030422 _bVLOAD _c201405060248 _dVLOAD _y201402171119 _zstaff
040			_aMX-SnUAN _bspa _cMX-SnUAN _erda
050		4	_aQB460-466
100	1		_aBecker, Werner. _eeditor. _9334586
245	1	0	_aNeutron Stars and Pulsars / _cedited by Werner Becker.
264		1	_aBerlin, Heidelberg : _bSpringer Berlin Heidelberg, _c2009.
300			_brecurso en línea.
336			_atexto _btxt _2rdacontent
337			_acomputadora _bc _2rdamedia
338			_arecurso en línea _bcr _2rdacarrier
347			_aarchivo de texto _bPDF _2rda
490	0		_aAstrophysics and Space Science Library, _x0067-0057 ; _v357
500			_aSpringer eBooks
505	0		_aRadio Pulsar Statistics -- Radio Emission Properties of Pulsars -- Rotating Radio Transients -- Intermittent Pulsars -- The Double Pulsar: A Unique Lab for Relativistic Plasma Physics and Tests of General Relativity -- X-Ray Emission from Pulsars and Neutron Stars -- Isolated Neutron Stars: The Challenge of Simplicity -- Millisecond Pulsars in Globular Clusters and the Field -- Theory of Radiative Transfer in Neutron Star Atmospheres and Its Applications -- Neutron Star Interiors and the Equation of State of Superdense Matter -- Neutron Star Cooling: I -- Neutron Star Cooling: II -- Turning Points in the Evolution of Isolated Neutron Stars'Magnetic Fields -- Pulsar Spin, Magnetic Fields, and Glitches -- Pulsar Emission: Where to Go -- The Theory of Pulsar Winds and Nebulae -- Implications of HESS Observations of Pulsar -- High Energy Emission from Pulsars and Pulsar Wind Nebulae -- High-energy Emission from the Polar Cap and Slot Gap -- Physics of Drifting Sub-pulses in Radio Pulsars -- Soft Gamma-Ray Repeaters and Magnetars -- X-Ray Polarimetry and Its Potential Use for Understanding Neutron Stars -- GeV Gamma-Ray Pulsar Detection -- Gravitational Waves from Spinning Neutron Stars.
520			_aNeutron stars are the most compact astronomical objects in the universe which are accessible by direct observation. Studying neutron stars means studying physics in regimes unattainable in any terrestrial laboratory. Understanding their observed complex phenomena requires a wide range of scientific disciplines, including the nuclear and condensed matter physics of very dense matter in neutron star interiors, plasma physics and quantum electrodynamics of magnetospheres, and the relativistic magneto-hydrodynamics of electron-positron pulsar winds interacting with some ambient medium. Not to mention the test bed neutron stars provide for general relativity theories, and their importance as potential sources of gravitational waves. It is this variety of disciplines which, among others, makes neutron star research so fascinating, not only for those who have been working in the field for many years but also for students and young scientists. The aim of this book is to serve as a reference work which not only reviews the progress made since the early days of pulsar astronomy, but especially focuses on questions such as: "What have we learned about the subject and how did we learn it?", "What are the most important open questions in this area?" and "What new tools, telescopes, observations, and calculations are needed to answer these questions?". All authors who have contributed to this book have devoted a significant part of their scientific careers to exploring the nature of neutron stars and understanding pulsars. Everyone has paid special attention to writing educational comprehensive review articles with the needs of beginners, students and young scientists as potential readers in mind. This book will be a valuable source of information for these groups.
590			_aPara consulta fuera de la UANL se requiere clave de acceso remoto.
710	2		_aSpringerLink (Servicio en línea) _9299170
776	0	8	_iEdición impresa: _z9783540769644
856	4	0	_uhttp://remoto.dgb.uanl.mx/login?url=http://dx.doi.org/10.1007/978-3-540-76965-1 _zConectar a Springer E-Books (Para consulta externa se requiere previa autentificación en Biblioteca Digital UANL)
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