000			03807nam a22004695i 4500
001			978-3-642-18418-5
003			DE-He213
005			20140220083256.0
007			cr nn 008mamaa
008			120217s2012 gw | s |||| 0|eng d
020			_a9783642184185 _9978-3-642-18418-5
024	7		_a10.1007/978-3-642-18418-5 _2doi
050		4	_aQB4
072		7	_aPG _2bicssc
072		7	_aSCI004000 _2bisacsh
072		7	_aNAT033000 _2bisacsh
082	0	4	_a520 _223
100	1		_aMiglio, Andrea. _eeditor.
245	1	0	_aRed Giants as Probes of the Structure and Evolution of the Milky Way _h[electronic resource] / _cedited by Andrea Miglio, Josefina Montalbán, Arlette Noels.
264		1	_aBerlin, Heidelberg : _bSpringer Berlin Heidelberg, _c2012.
300			_aXIV, 182p. 74 illus., 17 illus. in color. _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		_aPart I Asteroseismology of red giants -- Aspects of observational red giant population seismology -- Asteroseismology of red giants as a tool for studying stellar populations: first steps -- Adiabatic solar-like oscillations in red giant stars -- Energetic aspects of non-radial solar-like oscillations in red giants -- Part II Internal structure, atmosphere, and evolution of red giants: current models and their uncertainties -- Evolution and internal structure of red giants -- Uncertainties and systematics in stellar evolution models of Red Giant Stars -- Convection modelling and the morphology of RGBs in stellar clusters -- Helium burning in moderate-mass stars -- Hydrodynamic simulations of shell convection in stellar cores -- Impact of rotational mixing on the global and asteroseismic properties of red giants -- 3D picture of the convective envelope of a rotating RGB star -- Effects of rotation and thermohaline mixing in red giant stars -- 3D Model Atmospheres of Red Giant Stars -- Part III Stellar populations in the Milky Way -- Structure and Evolution of the Milky Way -- Red Giant stars: probing the MilkyWay chemical enrichment -- Chemical abundances of giants in globular clusters -- TRILEGAL, a TRIdimensional modeL of thE GALaxy: status and future -- The Besanc¸on model of stellar population synthesis of the Galaxy.
520			_aExciting results are blooming, thanks to a convergence between unprecedented asteroseismic data obtained by the satellites CoRoT and KEPLER, and state-of-the-art models of the internal structure of red giants and of galactic evolution. The pulsation properties now available for thousands of red giants promise to add valuable and independent constraints to current models of structure and evolution of our galaxy. Such a close connection between these domains opens a new very promising gate in our understanding of stars and galaxies. In this book international leaders in the field offer a wide perspective of the recent advancements in: Asteroseismology of red giants Models of the atmosphere, internal structure, and evolution of red giants Stellar population synthesis and models of the Milky Way
650		0	_aPhysics.
650	1	4	_aPhysics.
650	2	4	_aAstronomy, Observations and Techniques.
650	2	4	_aAstrophysics and Astroparticles.
700	1		_aMontalbán, Josefina. _eeditor.
700	1		_aNoels, Arlette. _eeditor.
710	2		_aSpringerLink (Online service)
773	0		_tSpringer eBooks
776	0	8	_iPrinted edition: _z9783642184178
830		0	_aAstrophysics and Space Science Proceedings, _x1570-6591
856	4	0	_uhttp://dx.doi.org/10.1007/978-3-642-18418-5
912			_aZDB-2-PHA
999			_c101898 _d101898