000			03827nam a22003975i 4500
001			302773
003			MX-SnUAN
005			20160429155759.0
007			cr nn 008mamaa
008			150903s2012 gw | o |||| 0|eng d
020			_a9783642184185 _99783642184185
024	7		_a10.1007/9783642184185 _2doi
035			_avtls000356483
039		9	_a201509030531 _bVLOAD _c201405060406 _dVLOAD _y201402191220 _zstaff
040			_aMX-SnUAN _bspa _cMX-SnUAN _erda
050		4	_aQB4
100	1		_aMiglio, Andrea. _eeditor. _9341157
245	1	0	_aRed Giants as Probes of the Structure and Evolution of the Milky Way / _cedited by Andrea Miglio, Josefina Montalbán, Arlette Noels.
264		1	_aBerlin, Heidelberg : _bSpringer Berlin Heidelberg, _c2012.
300			_axiv, 182 páginas 74 ilustraciones, 17 ilustraciones en color. _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 Proceedings, _x1570-6591
500			_aSpringer eBooks
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
590			_aPara consulta fuera de la UANL se requiere clave de acceso remoto.
700	1		_aMontalbán, Josefina. _eeditor. _9341158
700	1		_aNoels, Arlette. _eeditor. _9341159
710	2		_aSpringerLink (Servicio en línea) _9299170
776	0	8	_iEdición impresa: _z9783642184178
856	4	0	_uhttp://remoto.dgb.uanl.mx/login?url=http://dx.doi.org/10.1007/978-3-642-18418-5 _zConectar a Springer E-Books (Para consulta externa se requiere previa autentificación en Biblioteca Digital UANL)
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999			_c302773 _d302773