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[null,"1.","Record Nr.",null,"UNINA9910156169503321"]
[null,null,"Autore",null,"Soileau Jeanne Pitre"]
[null,null,"Titolo",null,"Yo' mama, Mary Mack, and Boudreaux and Thibodeaux : Louisiana children's folklore and play / / Jeanne Pitre Soileau"]
[null,null,"Pubbl/distr/stampa",null,"Jackson : , : University Press of Mississippi, , 2018"]
[null,null,"ISBN",null,"1-4968-1042-2"]
[null,null,"Descrizione fisica",null,"1 online resource (174 pages)"]
[null,null,"Collana",null,"Folklore Studies in a Multicultural World"]
[null,null,"Disciplina",null,"398.209763"]
[null,null,"Soggetti",null,"Folklore - Louisiana - History and criticism"]
[{"$nulls":4},"African Americans - History"]
[{"$nulls":4},"Children's literature, American - History and criticism"]
[{"$nulls":4},"Folklore and history - Louisiana"]
[{"$nulls":4},"New Orleans (La.) Race relations History 20th century"]
[null,null,"Lingua di pubblicazione",null,"Inglese"]
[null,null,"Formato",null,"Materiale a stampa"]
[null,null,null,"Livello bibliografico","Monografia"]
[null,null,null,"Note generali","Previously issued in print: 2016."]
[null,null,null,"Nota di bibliografia","Includes bibliographical references and index."]
[null,null,null,"Sommario/riassunto","'Yo' Mama, Mary Mack, and Boudreaux and Thibodeaux' presents a 44 year study of South Louisiana African American children's performance lore, from the last third of the twentieth century to the first ten years of the twenty-first, beginning with the era of integration in New Orleans and ending with the age of computers and the internet."]
[null,"2.","Record Nr.",null,"UNINA9910144720303321"]
[null,null,"Autore",null,"Stahler Steven William"]
[null,null,"Titolo",null,"The formation of stars : Steven W. Stahler and Francesco Palla"]
[null,null,"Pubbl/distr/stampa",null,"Weinheim, : Wiley-VCH, c2004"]
[null,null,"ISBN",null,"1-281-76453-1"]
[{"$nulls":4},"9786611764531"]
[{"$nulls":4},"3-527-61867-8"]
[{"$nulls":4},"3-527-61868-6"]
[null,null,"Descrizione fisica",null,"1 online resource (xiii, 852 p.)"]
[null,null,"Disciplina",null,"520"]
[{"$nulls":4},"523.8/8"]
[{"$nulls":4},"523.88"]
[null,null,"Soggetti",null,"Stars - Formation"]
[{"$nulls":4},"Stars - Evolution"]
[null,null,"Lingua di pubblicazione",null,"Inglese"]
[null,null,"Formato",null,"Materiale a stampa"]
[null,null,null,"Livello bibliografico","Monografia"]
[null,null,null,"Note generali","Description based upon print version of record."]
[null,null,null,"Nota di bibliografia","Includes bibliographical references and index."]
[null,null,"Nota di contenuto",null,"The Formation of Stars; Contents; Preface; I Star Formation in Our Galaxy; 1 Overview; 1.1 Stellar Nurseries:Orion; 1.2 Stellar Nurseries: Taurus-Auriga; 1.3 Stars and Their Evolution; 1.4 The Galactic Context; 2 The Interstellar Medium; 2.1 Galactic Gas and Its Detection; 2.2 Phases of the Interstellar Medium; 2.3 Interstellar Dust: Extinction and Thermal Emission; 2.4 Interstellar Dust: Properties of the Grains; 3 Molecular Clouds; 3.1 Giant Molecular Clouds; 3.2 Virial Theorem Analysis; 3.3 Dense Cores and Bok Globules; 4 Young Stellar Systems; 4.1 Embedded Clusters"]
[{"$nulls":4},"4.2 T and R Associations4.3 O B Associations; 4.4 Open Clusters; 4.5 The Initial Mass Function; II Physical Processes in Molecular Clouds; 5 Molecular Transitions: Basic Physics; 5.1 Interstellar Molecules; 5.2 Hydrogen (H2); 5.3 Carbon Monoxide (CO); 5.4 Ammonia (NH3); 5.5 Water (H2O); 5.6 Hydroxyl (OH); 6 Molecular Transitions: Applications; 6.1 Carbon Monoxide; 6.2 Ammonia; 6.3 Hydroxyl; 7 Heating and Cooling; 7.1 Cosmic Rays; 7.2 Interstellar Radiation; 7.3 Cooling by Atoms; 7.4 Cooling by Molecules and Dust; 8 Cloud Thermal Structure; 8.1 The Build up of Molecules"]
[{"$nulls":4},"8.2 The Molecular Interior8.3 Photodissociation Regions; 8.4 J-Shocks; 8.5 C-Shocks; III From Clouds to Stars; 9 Cloud Equilibrium and Stability; 9.1 Isothermal Spheres and the Jeans Mass; 9.2 Rotating "]
[{"$nulls":4},"Configurations; 9.3 Magnetic Flux Freezing; 9.4 Magnetostatic Configurations; 9.5 Support from MHD Waves; 10 The Collapse of Dense Cores; 10.1 Ambipolar Diffusion; 10.2 Inside-Out Collapse; 10.3 Magnetized Infall; 10.4 Rotational Effects; 11 Protostars; 11.1 First Core and Main Accretion Phase; 11.2 Interior Evolution: Deuterium Burning; 11.3 Protostellar Disks; 11.4 More Massive Protostars"]
[{"$nulls":4},"11.5 The Observational Search12 Multiple Star Formation; 12.1 Dynamical Fragmentation of Massive Clouds; 12.2 Young Binary Stars; 12.3 TheOrigin of Binaries; 12.4 Formation of Stellar Groups; 12.5 Massive Stars and Their Associations; IV Environmental Impact of Young Stars; 13 Jets and Molecular Outflows; 13.1 Jets from Embedded Stars; 13.2 Molecular Outflows; 13.3 Wind Generation: Pressure Effects; 13.4 Wind Generation: Rotation and Magnetic Fields; 13.5 Jet Propagation and Entrainment; 14 Interstellar Masers; 14.1 Observed Characteristics; 14.2 Maser Theory: Basic Principles"]
[{"$nulls":4},"14.3 Maser Theory: Further Considerations14.4 Tracing Jets and Outflows; 15 Effects of Massive Stars; 15.1 HII Regions; 15.2 Ultracompact HII Regions and Hot Cores; 15.3 Winds and Molecular Outflows; 15.4 Photoevaporation of Gas; 15.5 Induced Star Formation; V Pre-Main-Sequence Stars; 16 Quasi-Static Contraction; 16.1 The Stellar Birthline; 16.2 The Contraction Process; 16.3 Nuclear Reactions; 16.4 Brown Dwarfs; 16.5 Spinup and Spindown; 17 T Tauri Stars; 17.1 Line and Continuum Emission; 17.2 Outflow and Infall; 17.3 Circumstellar Disks; 17.4 Temporal Variability"]
[{"$nulls":4},"17.5 Post-T Tauri Stars and Beyond"]
[null,null,null,"Sommario/riassunto","This book is a comprehensive treatment of star formation, one of the most active fields of modern astronomy. The reader is guided through the subject in a logically compelling manner. Starting from a general description of stars and interstellar clouds, the authors delineate the earliest phases of stellar evolution. They discuss formation activity not only in the Milky Way, but also in other galaxies, both now and in the remote past. Theory and observation are thoroughly integrated, with the aid of numerous figures and images. In summary, this volume is an invaluable resource, both as a text f"]