000 03235nam a22003735i 4500
001 304659
003 MX-SnUAN
005 20170705134304.0
007 cr nn 008mamaa
008 150903s2012 gw | o |||| 0|eng d
020 _a9783642224911
_99783642224911
024 7 _a10.1007/9783642224911
_2doi
035 _avtls000357448
039 9 _a201509030558
_bVLOAD
_c201405070216
_dVLOAD
_y201402191316
_zstaff
040 _aMX-SnUAN
_bspa
_cMX-SnUAN
_erda
050 4 _aQB1-991
100 1 _aMatteucci, Francesca.
_eautor
_9343561
245 1 0 _aChemical Evolution of Galaxies /
_cby Francesca Matteucci.
264 1 _aBerlin, Heidelberg :
_bSpringer Berlin Heidelberg :
_bImprint: Springer,
_c2012.
300 _axiii, 225 páginas 128 ilustraciones, 68 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 _aAstronomy and Astrophysics Library,
_x0941-7834
500 _aSpringer eBooks
505 0 _aIntroduction -- Basic Ingredients for Modelling Chemical Evolution -- Simple Models of Chemical Evolution -- Numerical Models of Chemical Evolution -- Chemical Evolution of the Milky Way and other Spirals -- Chemical Evolution of Early Type Galaxies -- Chemical Evolution of Irregular Galaxies -- Cosmic Chemical Evolution -- Acronyms.
520 _aThe term “chemical evolution of galaxies” refers to the evolution of abundances of chemical species in galaxies, which is due to nuclear processes occurring in stars and to gas flows into and out of galaxies. This book deals with the chemical evolution of galaxies of all morphological types (ellipticals, spirals and irregulars) and stresses the importance of the star formation histories in determining the properties of stellar populations in different galaxies. The topic is approached in a didactical and logical manner via galaxy evolution models which are compared with observational results obtained in the last two decades: The reader is given an introduction to the concept of chemical abundances and learns about the main stellar populations in our Galaxy as well as about the classification of galaxy types and their main observables. In the core of the book, the construction and solution of chemical evolution models are discussed in detail, followed by descriptions and interpretations of observations of the chemical evolution of the Milky Way, spheroidal galaxies, irregular galaxies and of cosmic chemical evolution. The aim of this book is to provide an introduction to students as well as to amend our present ideas in research; the book also summarizes the efforts made by authors in the past several years in order to further future research in the field.
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:
_z9783642224904
856 4 0 _uhttp://remoto.dgb.uanl.mx/login?url=http://dx.doi.org/10.1007/978-3-642-22491-1
_zConectar a Springer E-Books (Para consulta externa se requiere previa autentificación en Biblioteca Digital UANL)
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999 _c304659
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