Starburst

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Starburst Galaxies: Near and Far

Author : L. Tacconi,D. Lutz
Publisher : Springer Science & Business Media
Page : 349 pages
File Size : 51,9 Mb
Release : 2012-12-06
Category : Science
ISBN : 9783642565380

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Starburst Galaxies: Near and Far by L. Tacconi,D. Lutz Pdf

A major fraction of star formation in the universe occurs in starbursts. These regions of particularly rapid star formation are often located towards the centers of host galaxies. Studies of this kind of star formation at high redshift have produced astonishing results over recent years that were only possible with the latest generation of large ground-based and space telescopes. The papers collected in this volume present these results in the context of the much firmer foundation of star formation in the local universe, and they emphasize all the important topics, from star formation in different environments to the cosmic star formation history.

Advanced Lectures on the Starburst-AGN Connection

Author : D. Kunth
Publisher : World Scientific
Page : 396 pages
File Size : 42,8 Mb
Release : 2001
Category : Science
ISBN : 9810246161

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Advanced Lectures on the Starburst-AGN Connection by D. Kunth Pdf

A group of leading experts in the field of starbursts and active galactic nuclei have joined hands to produce this review volume which covers the starburst-AGN connection, and the tests to be carried out with the upcoming new astronomical facilities to ascertain the relevance of both components to the formation and evolution of galaxies.The book is addressed to advanced graduate students and researchers in the fields of active galactic nuclei and young galaxies.

Massive Stars in Starbursts

Author : Claus Leitherer,Space Telescope Science Institute (U.S.)
Publisher : Cambridge University Press
Page : 354 pages
File Size : 43,7 Mb
Release : 1991-05-16
Category : Science
ISBN : 0521404657

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Massive Stars in Starbursts by Claus Leitherer,Space Telescope Science Institute (U.S.) Pdf

This book reviews the importance of massive stars in several areas of astrophysics. Massive stars are objects that are 10-100 times the mass of our Sun. Above ten solar masses, loss through stellar winds begins to have a major impact on the evolution of a star. The upper limit of 100 solar masses is derived from observations. Significant progress has now been achieved in massive star research. New models, along with high quality observations, have improved our understanding of the formation, structure, atmosphere, and evolution of these massive objects. They are formed in violent bursts of star formation and are probably related to the phenomena observed in active galactic nuclei. The workshop at the Space Telescope Science Institute examined the interplay between the astrophysics of massive stars and their location in extragalactic starburst regions. There are eighteen chapters by leading researchers. Each has been carefully edited to ensure that the book is a comprehensive introduction to the theory and observation of massive stars in starburst regions.

Starbursts

Author : Richard de Grijs,Rosa M. González Delgado
Publisher : Springer Science & Business Media
Page : 390 pages
File Size : 49,7 Mb
Release : 2006-05-11
Category : Science
ISBN : 9781402035395

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Starbursts by Richard de Grijs,Rosa M. González Delgado Pdf

Starbursts are important features of early galaxy evolution. Many of the distant, high-redshift galaxies we are able to detect are in a starbursting phase, often apparently provoked by a violent gravitational interaction with another galaxy. In fact, if we did not know that major starbursts existed, these conference proceedings testify that we would indeed have difficulties explaining the key properties of the Universe! These conference proceedings cover starbursts from the small-scale star-forming regions in nearby galaxies to galaxy-wide events at high redshifts; one of the major themes of the conference proved to be "scalability", i.e., can we scale up the small-scale events to describe the physics on larger scales. The key outcome of this meeting – and these proceedings – is a resounding "yes" to this fundamental, yet profound question. The enhanced synergy facilitated by the collaboration among observers using cutting-edge ground and space-based facilities, theorists and modellers has made these proceedings a true reflection of the state of the art in this very rapidly evolving field.

Starbursts and Galaxy Evolution

Author : Xuan Thuan Trinh,Thierry Montmerle,J. Thanh Van Tran
Publisher : Atlantica Séguier Frontières
Page : 626 pages
File Size : 48,7 Mb
Release : 1987
Category : Galaxies
ISBN : 2863320505

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Starbursts and Galaxy Evolution by Xuan Thuan Trinh,Thierry Montmerle,J. Thanh Van Tran Pdf

Starbursts Triggers, Nature, and Evolution

Author : Bruno Guiderdoni
Publisher : Springer
Page : 264 pages
File Size : 49,9 Mb
Release : 2013-11-11
Category : Science
ISBN : 9783662297421

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Starbursts Triggers, Nature, and Evolution by Bruno Guiderdoni Pdf

Starbursts are regions of unusually rapid star formation, often located in the central parts of galaxies. They differ from more normal regions of star formation in terms of the throughput of mass and the rapidity with which the gas is consumed. In the last twenty years, extensive observational data at most wavelengths have become available on starbursts, but many important issues remain to be addressed, observationally as well as theoretically. How are strong episodes of star formation triggered? What is the quantity of gas converted into stars during bursts? What is the initial mass function of stars in these events? How does the feedback from stars influence the interstellar medium and self-regulate star formation? What is the subsequent chemical and photometric evolution? How do starbursts rule the formation and evolution of galaxies? In recent years, many observational data at different wavelengths (optical, radio, infrared, X-ray) have become available. However, these observations are still fragmentary in the sense that different classes of objects have been observed in different ways, and the coverage is not consistently deep or complete. As a consequence, an overall observational picture of starburst galaxies is missing, and theoretical understanding and modelling have remained highly tentative. The purpose of the school Starbursts: Triggers, Nature, and Evolution was to gather theorists and observers with complementary approaches to the starburst phenomenon, in order to summarize the state-of-the-art of the observations and models, emphasizing the consistency of the various viewpoints.

Craft: Volume 01

Author : Carla Sinclair
Publisher : "O'Reilly Media, Inc."
Page : 168 pages
File Size : 52,7 Mb
Release : 2006-11-28
Category : Crafts & Hobbies
ISBN : 0596529287

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Craft: Volume 01 by Carla Sinclair Pdf

CRAFT is the first project-based magazine dedicated to the renaissance that is occurring within the world of crafts. Celebrating the DIY spirit, CRAFT's goal is to unite, inspire, inform and entertain a growing community of highly imaginative people who are transforming traditional art and crafts with unconventional, unexpected and even renegade techniques, materials and tools; resourceful spirits who undertake amazing crafting projects in their homes and communities. Volume 01, the premier issue, features 23 projects with a twist! Make a programmable LED shirt, turn dud shoes into great knitted boots, felt an iPod cocoon, embroider a skateboard, and much more.

Data Mesh

Author : Zhamak Dehghani
Publisher : "O'Reilly Media, Inc."
Page : 387 pages
File Size : 45,7 Mb
Release : 2022-03-08
Category : Computers
ISBN : 9781492092360

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Data Mesh by Zhamak Dehghani Pdf

Many enterprises are investing in a next-generation data lake, hoping to democratize data at scale to provide business insights and ultimately make automated intelligent decisions. In this practical book, author Zhamak Dehghani reveals that, despite the time, money, and effort poured into them, data warehouses and data lakes fail when applied at the scale and speed of today's organizations. A distributed data mesh is a better choice. Dehghani guides architects, technical leaders, and decision makers on their journey from monolithic big data architecture to a sociotechnical paradigm that draws from modern distributed architecture. A data mesh considers domains as a first-class concern, applies platform thinking to create self-serve data infrastructure, treats data as a product, and introduces a federated and computational model of data governance. This book shows you why and how. Examine the current data landscape from the perspective of business and organizational needs, environmental challenges, and existing architectures Analyze the landscape's underlying characteristics and failure modes Get a complete introduction to data mesh principles and its constituents Learn how to design a data mesh architecture Move beyond a monolithic data lake to a distributed data mesh.

The Neutral ISM in Starburst Galaxies

Author : Susanne Aalto,Susanne Hüttemeister,Alan Pedlar
Publisher : Unknown
Page : 412 pages
File Size : 54,8 Mb
Release : 2004
Category : Science
ISBN : UOM:39015061470814

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The Neutral ISM in Starburst Galaxies by Susanne Aalto,Susanne Hüttemeister,Alan Pedlar Pdf

Trino: The Definitive Guide

Author : Matt Fuller,Manfred Moser,Martin Traverso
Publisher : "O'Reilly Media, Inc."
Page : 310 pages
File Size : 41,5 Mb
Release : 2021-04-14
Category : Computers
ISBN : 9781098107680

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Trino: The Definitive Guide by Matt Fuller,Manfred Moser,Martin Traverso Pdf

Perform fast interactive analytics against different data sources using the Trino high-performance distributed SQL query engine. With this practical guide, you'll learn how to conduct analytics on data where it lives, whether it's Hive, Cassandra, a relational database, or a proprietary data store. Analysts, software engineers, and production engineers will learn how to manage, use, and even develop with Trino. Initially developed by Facebook, open source Trino is now used by Netflix, Airbnb, LinkedIn, Twitter, Uber, and many other companies. Matt Fuller, Manfred Moser, and Martin Traverso show you how a single Trino query can combine data from multiple sources to allow for analytics across your entire organization. Get started: Explore Trino's use cases and learn about tools that will help you connect to Trino and query data Go deeper: Learn Trino's internal workings, including how to connect to and query data sources with support for SQL statements, operators, functions, and more Put Trino in production: Secure Trino, monitor workloads, tune queries, and connect more applications; learn how other organizations apply Trino

The Brightest Binaries

Author : D. Vanbeveren,W. van Rensbergen,C. de Loore
Publisher : Springer Science & Business Media
Page : 360 pages
File Size : 48,8 Mb
Release : 2001-11-30
Category : Science
ISBN : 1402003765

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The Brightest Binaries by D. Vanbeveren,W. van Rensbergen,C. de Loore Pdf

The evolution of galaxies is governed mainly by the evolution of massive stars whereas the evolution of a massive star depends primarily on its mass, chemical composition and on whether or not the star is a Single object or a binary component. To study the evolution of galaxies, it is therefore essential to know how stellar masses are distributed at birth, how many stars are formed in binaries, and what the mass ratio and orbital period distribution of binaries look like. Massive stars are intrinsically the brightest stars, so that it may be possible to discover their properties in distant groups prOvided that large telescopes can be used for basic stellar observations. However, until now the observations of massive stars have been reasonably complete only for a small region of our own Galaxy (~ 3 kpc from the Sun). One hopes that the conclusions resulting from these observations hold for the whole Galaxy, for the whole cosmos. With 'The Brightest Stars' of De Jager (1980) in mind, the present monograph is an addendum and an update in which we discuss the observations of 'The Brightest Binaries' in the framework of stellar evolution. A small or intermediate mass star close to the Sun may look brighter than a massive one far away. However, within volume limited star samples, the massive stars are on average also the brightest ones. In the present monograph (similarly as in the work of De Jager), bright means massive. The book consists of four main chapters.

New Vision Of An Old Cluster, A - Untangling Coma Berenices

Author : Alain Mazure,Fabienne Casoli,Florence Durret,Daniel Gerbal
Publisher : World Scientific
Page : 246 pages
File Size : 48,5 Mb
Release : 1998-08-15
Category : Electronic
ISBN : 9789814545419

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New Vision Of An Old Cluster, A - Untangling Coma Berenices by Alain Mazure,Fabienne Casoli,Florence Durret,Daniel Gerbal Pdf

Together with Virgo, the Coma Berenices cluster is one of the most well-studied clusters at all wavelengths and in all aspects, from the Sunyaev-Zeldovich effect to star formation in galaxies. In a way, it is the prototype of rich clusters. Recent observational results, linked to the improvement of techniques such as X-ray and UV observations, along with multi-object spectroscopy, have shown that they could change our vision of this cluster. It is thus time for observers and theoreticians to confront all these new ideas and observations on the Coma cluster.The topics in this volume include: cosmological aspects of the Coma cluster, comparison with distant clusters; substructures; matter content and distribution; Sunyaev-Zeldovich effect; dynamical modelling, cluster dynamics; environmental effects on galaxies, star formation.

Windows on Galaxies

Author : Giuseppina Fabbiano,John S. Gallagher,Alvio Renzini
Publisher : Springer Science & Business Media
Page : 376 pages
File Size : 45,5 Mb
Release : 2012-12-06
Category : Science
ISBN : 9789400905436

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Windows on Galaxies by Giuseppina Fabbiano,John S. Gallagher,Alvio Renzini Pdf

Along with the traditional optical window, many new windows have been opened on galaxies in the last two decades, made possible by new developments in groundbased detectors and by space missions that allow detection of photons that are otherwise absorbed by the Earth's atmosphere. Galaxies can now be observed in the radio, submillimeter, IR, optical, UV, X- and gamma-ray bands, each window allowing us to learn more about galactic components and properties. These developments have also imposed the view that a deeper understanding of even normal galaxies requires a panchromatic approach, making use of all of the data gathered from the different windows to synthesize a comprehensive physical image of these complex astronomical systems. Windows on Galaxies presents a comprehensive view of galaxies through all the available windows, bringing together both theoretical and experimental approaches in the form of a series of reviews reporting the most recent developments complemented by contributed talks and discussions. TEXT NO. 2 The sixth workshop of the Advanced School of Astronomy examined galaxies through all available wavelength windows. Over the last twenty years, new wavelength windows have been opened in astronomy which have created many new possibilities for the observation of the properties of galaxies. The outcome of the meeting clearly stated that the approach towards the studying of galaxies should be panchromatic. Each window, from radio to gamma-rays, shows different components, and a synthesis of this knowledge presents astronomers with a comprehensive physical image of these astronomical systems: star formation, evolution of galaxies, molecular contents, gas flows, interstellar matter and properties of galaxies in the several wavelength fields are discussed in this volume.