000			03855nam a22004815i 4500
001			978-1-4020-5425-9
003			DE-He213
005			20260521092122.0
007			cr nn 008mamaa
008			100301s2007 ne | s |||| 0|eng d
020			_a9781402054259
020			_a99781402054259
024	7		_a10.1007/978-1-4020-5425-9 _2doi
082	0	4	_a520 _223
100	1		_aHARTQUIST, T.W. _eeditor.
245	1	0	_aDiffuse Matter from Star Forming Regions to Active Galaxies _h[electronic resource] : _bA Volume Honouring John Dyson / _cedited by T.W. HARTQUIST, J.M. PITTARD, S.A.E.G. FALLE.
264		1	_aDordrecht : _bSpringer Netherlands, _c2007.
300			_aXX, 342 p. _bonline resource.
336			_atext _btxt _2rdacontent
337			_acomputer _bc _2rdamedia
338			_aonline resource _bcr _2rdacarrier
347			_atext file _bPDF _2rda
490	1		_aAstrophysics and Space Science Proceedings, _x1570-6591
505	0		_aStar Forming Regions -- Numerical Simulations of Star Formation -- Molecular Astrophysics of Star Formation -- Dusty Plasma Effects in Star Forming Regions -- Massive Star Formation -- Spectropolarimetry and the Study of Circumstellar Disks -- How to Move Ionized Gas: An Introduction to the Dynamics of HII Regions -- MHD Ionization Fronts -- Herbig-Haro Jets from Young Stars -- Hypersonic Molecular Shocks in Star Forming Regions -- The Effects of Evolved Stars on Their Environments -- Wind-Blown Bubbles around Evolved Stars -- Do Fast Winds Dominate the Dynamics of Planetary Nebulae? -- Spectral Studies of Supernova Remnants -- Multicomponent Flows and Cosmic Rays -- Mass-Loaded Flows -- The Effects of Cosmic Rays on Interstellar Dynamics -- The Status of Observations and Speculations Concerning Ultra High-Energy Cosmic Rays -- Starburst Galaxies and Active Galactic Nuclei -- The Messier 82 Starburst Galaxy -- Active Galactic Nuclei.
520			_aJohn Dyson has contributed to the study of the hydrodynamic processes that govern a wide variety of astrophysical sources which he has helped explain. In this volume dedicated to him, introductory reviews to a number of the key processes and to the sources themselves are given by leading experts. The mechanisms in which the multi-component natures of media affect their dynamics receive particular attention, but the roles of hydromagnetic effects are also highlighted. The importance of cosmic ray moderation and mass transfer between different thermal phases for cosmic ray moderation and mass transfer between different thermal phases for the evolution of flows are amongst the topics treated. The main types of regions considered include those where stars form, the circumstellar environments of evolved stars, the larger scale interstellar structures caused by the mass loss of stars, and those where the lines of AGNs form. The reviews complement one another and together provide a coherent introduction to the astrophysics of diffuse sources suitable for postgraduate students and researchers in astrophysics. Individual reviews stand alone and are suitable for an audience that includes advanced undergraduates doing final year projects.
650		0	_aPHYSICS.
650		0	_aASTRONOMY.
650		0	_aASTROPHYSICS.
650	1	4	_aPHYSICS.
650	2	4	_aASTRONOMY, ASTROPHYSICS AND COSMOLOGY.
650	2	4	_aASTRONOMY.
650	2	4	_aASTROPHYSICS.
700	1		_aPITTARD, J.M. _eeditor.
700	1		_aFALLE, S.A.E.G. _eeditor.
710	2		_aSpringerLink (Online service)
773	0		_tSpringer eBooks
776	0	8	_iPrinted edition: _z9781402054242
830		0	_aAstrophysics and Space Science Proceedings, _x1570-6591
856	4	0	_uhttp://dx.doi.org/10.1007/978-1-4020-5425-9 _zVer el texto completo en las instalaciones del CICY
912			_aZDB-2-PHA
942			_2ddc _cER
999			_c37201 _d37201