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    [name] => Globular Clusters: Jewels to Trace the Structure of Galaxies
    [meta_title] => Globular Clusters: Jewels to Trace the Structure of Galaxies 9786070268106 libro
    [meta_description] => Globular Clusters: Jewels to Trace the Structure of Galaxies 9786070268106 libro
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    [image_label] => Globular Clusters: Jewels to Trace the Structure of Galaxies
    [small_image_label] => Globular Clusters: Jewels to Trace the Structure of Galaxies
    [thumbnail_label] => Globular Clusters: Jewels to Trace the Structure of Galaxies
    [author] => Álamo Martínez, Karla Adriana
    [language] => Inglés
    [number_pages] => 145
    [size] => 14 x 21
    [finished] => Rústico
    [isxn] => 9786070268106
    [weight_mb] => 0.246
    [edition_data] => 1a edición, año de edición -2015-
    [topic] => Física y astronomía
    [price] => 506.0000
    [weight] => 0.2460
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    [description] => Los cúmulos globulares son sistemas estelares viejos, muy densos y trazadores de la estructura galáctica. En este libro se muestran los sistemas de cúmulos globulares en tres grupos fósiles. Al utilizar datos del telescopio espacial Hubble, durante el desarrollo de esta investigación, se encontró que la distribución espacial, de color y frecuencia específica de los cúmulos globulares, es similar a la de elípticas en cúmulos.
    [short_description] => "...ha demostrado cómo la relación entre los cúmulos globulares y la materia oscura depende de la distancia desde el centro del grupo de galaxias".
    [meta_keyword] => Globular Clusters: Jewels to Trace the Structure of Galaxies, Física y astronomía, Coordinación de Estudios de Posgrado
    [author_bio] => 
Álamo Martínez, Karla Adriana 	
Cursó la licenciatura en Física en la Universidad de Guanajuato, donde obtuvo el grado con el trabajo: "Dinámica de las galaxias más brillantes de cúmulos ricos", dirigido por el doctor Heinz Andernach; tesis merecedora del "Premio Luis Enrique Erro" que se otorga en el marco del Congreso Nacional de Astronomía (2008). En 2009 cursó la maestría en Ciencias (Astronomía) en el Centro de Radioastronomía y Astrofísica de la Universidad Nacional Autónoma de México. Entre 2009 y 2012 realizó estancias de investigación en el Observatorio Europeo Austral (Chile) y en el Herzberg Institute for Astrophysics (Canadá). En 2014 obtuvo el grado de Doctora en Ciencias (Astrofísica) con la investigación que aquí se presenta y que estuvo dirigida por los doctores Rosa A. González Lópezlira y John Blakeslee. Actualmente tiene una posición posdoctoral del Fondo Nacional Científico y Tecnológico en Santiago de Chile.
    [toc] => 1. Globular Clusters ... 1.1 Individual Properties... 1.1.1 Size... 1.1.2 Color Magnitude Diagram... 1.1.3 Ages... 1.1.4 Structure and Dynamics... 1.1.5 Stellar Content ... 1.2 Globular Cluster System Properties... 1.2.1 Specific Frequency... 1.2.2 Color Distribution... 1.2.3 Luminosity Function... 1.2.4 Intergalactic Globular Clusters...2 Galaxy Formation and Evolution... 2.1 Light Distribution... 2.1.1 Surface Brightness Profiles... 2.1.2 Luminosity Function... 2.2 Galaxy Content... 2.2.1 Initial Mass Function... 2.2.2 Dark Matter... 2.3 Galaxy Formation Scenarios... 2.3.1 Monolithic Collapse... 2.3.2 Hierarchical Assembly... Globular Clusters: Jewels to Trace the Structure of Galaxies... 2.4 Standard Paradigm... 2.5 This Thesis... 3 Fossil Groups... 3.1 Description.... 3.2 The Sample... 3.2.1 NGC 6482... 3.2.2 NGC 1132... 3.2.3 ESO 306-G017.... 3.3 Observations and Data Reduction... 3.4 Analysis... 3.4.1 Surface Brightness... 3.4.2 GC Detection... 3.5 Results... 3.5.1 Globular Cluster Color Distribution... 3.5.2 Globular Cluster Spatial Distribution... 3.5.3 Globular Cluster Luminosity Function... 3.5.4 Specific Frequency... 3.6 Discussion... 3.6.1 Comparison with Cluster Ellipticals... 3.6.2 Comparisons with X-ray Data... 4 Abell 1689... 4.1 Description... 4.2 Observations and Data Reduction... 4.3 Analysis... 4.3.1 Galaxy Modeling... 4.3.2 Object Detection... 4.3.3 GC Candidate Selection... 4.3.4 Completeness... 4.3.5 Background Contamination... 4.4 Results and Discussion... 4.4.1 Total GC Number and Specific Frequency...4.4.2 Comparison of Mass Profiles...4.5 Modeling of Individual Galaxies...5 Conclusions...5.1 Fossil Groups... 5.2 Abell 1689... Bibliography.
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