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The Birth of Star Clusters

Author : Steven Stahler

Publisher : Springer

Page : 205 pages

File Size : 16,63 MB

Release : 2017-11-04

Category : Science

ISBN : 3319228013

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Book Description

All stars are born in groups. The origin of these groups has long been a key question in astronomy, one that interests researchers in star formation, the interstellar medium, and cosmology. This volume summarizes current progress in the field, and includes contributions from both theorists and observers. Star clusters appear with a wide range of properties, and are born in a variety of physical conditions. Yet the key question remains: How do diffuse clouds of gas condense into the collections of luminous objects we call stars? This book will benefit graduate students, newcomers to the field, and also experienced scientists seeking a convenient reference.



Information & On-Line Data in Astronomy

Author : D Egret

Publisher : Springer Science & Business Media

Page : 291 pages

File Size : 20,81 MB

Release : 2012-12-06

Category : Mathematics

ISBN : 9401103976

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Book Description

The ability of storing, managing, and giving access to the huge quantity of data collected by astronomical observatories is one of the major challenges of modern astronomy. At the same time, the growing complexity of data systems implies a change of concepts: the scientist has to manipulate data as well as information. Recent developments of the `WorldWideWeb' bring interesting answers to these problems. The book presents a wide selection of databases, archives, data centers, and information systems. Clear and up-to-date descriptions are included, together with their scientific context and motivations. Audience: This volume provides an essential tool for astronomers, librarians, data specialists and computer engineers.



Dynamics of Young Star Clusters and Associations

Author : Cathie Clarke

Publisher : Springer

Page : 356 pages

File Size : 47,8 MB

Release : 2015-09-11

Category : Science

ISBN : 3662472902

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Book Description

Where do most stars (and the planetary systems that surround them) in the Milky Way form? What determines whether a young star cluster remains bound (such as an open or globular cluster), or disperses to join the field stars in the disc of the Galaxy? These questions not only impact understanding of the origins of stars and planetary systems like our own (and the potential for life to emerge that they represent), but also galaxy formation and evolution, and ultimately the story of star formation over cosmic time in the Universe. This volume will help readers understand our current views concerning the answers to these questions as well as frame new questions that will be answered by the European Space Agency's Gaia satellite that was launched in late 2013. The book contains the elaborated notes of lectures given at the 42nd Saas-Fee Advanced Course “Dynamics of Young Star Clusters & Associations" by Cathie Clarke (University of Cambridge) who presents the theory of star formation and dynamical evolution of stellar systems, Robert Mathieu (University of Wisconsin) who discusses the kinematics of star clusters and associations, and I. Neill Reid (S pace Telescope Science Institute) who provides an overview of the stellar populations in the Milky Way and speculates on from whence came the Sun. As part of the Saas-Fee Advanced Course Series, the book offers an in-depth introduction to the field serving as a starting point for Ph.D. research and as a reference work for professional astrophysicists.



The Evolution of The Milky Way

Author : Francesca Matteucci

Publisher : Springer Science & Business Media

Page : 605 pages

File Size : 13,35 MB

Release : 2012-12-06

Category : Science

ISBN : 9401009384

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Book Description

This review of the most up-to-date observational and theoretical information concerning the chemical evolution of the Milky Way compares the abundances derived from field stars and clusters, giving information on the abundances and dynamics of gas.



Observer’s Guide to Star Clusters

Author : Mike Inglis

Publisher : Springer Science & Business Media

Page : 294 pages

File Size : 21,9 MB

Release : 2013-07-20

Category : Science

ISBN : 1461475678

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Book Description

Amateur astronomers of all expertise from beginner to experienced will find this a thorough star cluster atlas perfect for easy use at the telescope or through binoculars. It enables practical observers to locate the approximate positions of objects in the sky, organized by constellation. This book was specifically designed as an atlas and written for easy use in field conditions. The maps are in black-and-white so that they can be read by the light of a red LED observer’s reading light. The clusters and their names/numbers are printed in bold black, against a “grayed-out” background of stars and constellation figures. To be used as a self-contained reference, the book provides the reader with detailed and up-to-date coverage of objects visible with small-, medium-, and large-aperture telescopes, and is equally useful for simple and computer-controlled telescopes. In practice, GO-TO telescopes can usually locate clusters accurately enough to be seen in a low-magnification eyepiece, but this of course first requires that the observer knows what is visible in the sky at a given time and from a given location, so as to input a locatable object. This is where "The Observer's Guide to Star Clusters" steps in as an essential aid to finding star clusters to observe and an essential piece of equipment for all amateur astronomers.



Observing and Cataloguing Nebulae and Star Clusters

Author : Wolfgang Steinicke

Publisher : Cambridge University Press

Page : 661 pages

File Size : 10,94 MB

Release : 2010-08-19

Category : Science

ISBN : 1139490109

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Book Description

Providing the first comprehensive historical study of the New General Catalogue, this book is an important resource to all those interested in the history of modern astronomy and visual deep-sky observing. It covers the people, observatories, instruments and methods involved in nineteenth-century visual deep-sky observing, as well as prominent deep-sky objects.



Star Clusters and How to Observe Them

Author : Mark Allison

Publisher : Springer Science & Business Media

Page : 218 pages

File Size : 22,77 MB

Release : 2006-04-04

Category : Science

ISBN : 1846281989

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Book Description

Astronomy enthusiasts will all appreciate the detailed yet easily-assimilated description of star clusters, how they were formed as our Milky Way galaxy, how they evolved, and how they are classified. The latest research has revealed a vast amount of fascinating information about the clusters, along with some spectacular photographs. Modern commercially-made telescopes enable amateur astronomers to see a surprising amount of detail, and to record – using CCD cameras, video, webcams or even film – some remarkably beautiful and detailed images. Contained here also is detailed information on using refractors, reflectors, and, of course, Meade and Celestron’s ubiquitous range of computer-controlled SCT telescopes.



Handbook of Star Forming Regions: The northern sky

Author : Bo Reipurth

Publisher :

Page : 0 pages

File Size : 44,24 MB

Release : 2008

Category : Northern sky (Astronomy)

ISBN : 9781583816707

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Book Description

The Handbook describes the 6̃0 most important star forming regions within approximately 2 kpc, and has been written by a team of 105 authors with expertise in the individual regions. It consists of two full-color volumes, one for the northern and one for the southern hemisphere, with a total of over 1900 pages. The Handbook is full of stunning color images from some of the best astrophotographers, complementing the extensive research, figures, and tables presented by the authors. These volumes aim to be a source of comprehensive factual information about each region, with extensive references to the literature. A useful reference guide for both researchers and students, the Handbook provides a unique and detailed presentation of our current knowledge about the nearest and most important star forming regions.



Astrophysical Data

Author : Kenneth R. Lang

Publisher : Springer Science & Business Media

Page : 942 pages

File Size : 30,40 MB

Release : 2012-12-06

Category : Science

ISBN : 146840640X

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Book Description

This volume of Astrophysical Data deals with Planets and Stars; a second volume, Part II, will give data for Galaxies and the Universe. They both pro vide basic data for use by all scientists, from the amateur astronomer to the professional astrophysicist. In this first volume, we not only provide physical parameters of planets, stars and their environment, but we also provide the celestial coordinates required to observe them. Here we use c.g.s. units, for they are the most commonly used in astron omy and astrophysics; but our volume begins with astronomical and physical constants and the conversion factors needed for other units. The next section concerns the planets and their satellites; it singles out the Earth and Moon for special treatment. Spacecraft rendezvous with the planets and satellites have led to improved values for their atmospheric compositions, orbital parameters, magnetic fields, masses, radii, rotation periods, and surface pressures and temperatures. This section also contains data for the asteroids, comets and their debris. We then discuss everyday stars, beginning with the Sun, and continuing with basic stellar data, the brightest stars and nearby stars. Special categories of stars, such as the Wolf-Rayet stars, magnetic stars, flare stars, and RS CVn binary stars, are included.



The Initial Mass Function 50 Years Later

Author : Edvige Corbelli

Publisher : Springer Science & Business Media

Page : 551 pages

File Size : 21,41 MB

Release : 2007-10-06

Category : Science

ISBN : 1402034075

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Book Description

Theideatocelebrate50yearsoftheSalpeterIMFoccurredduringtherecent IAU General Assembly in Sydney, Australia. Indeed, it was from Australia that in July 1954 Ed Salpeter submitted his famous paper "The Luminosity Function and Stellar Evolution" with the rst derivation of the empirical stellar IMF. This contribution was to become one of the most famous astrophysics papers of the last 50 years. Here, Ed Salpeter introduced the terms "original mass function" and "original luminosity function", and estimated the pro- bility for the creation of stars of given mass at a particular time, now known as the "Salpeter Initial Mass Function", or IMF. The paper was written at the Australian National University in Canberra on leave of absence from Cornell University (USA) and was published in 1955 as 7 page note in the Astroph- ical Journal Vol. 121, page 161. To celabrate the 50th anniversary of the IMF, along with Ed Salpeter’s 80th birthday, we have organized a special meeting that brought together scientists involved in the empirical determination of this fundamental quantity in a va- ety of astrophysical contexts and other scientists fascinated by the deep imp- cations of the IMF on star formation theories, on the physical conditions of the gas before and after star formation, and on galactic evolution and cosmology. The meeting took place in one of the most beautiful spots of the Tuscan countryside, far from the noise and haste of everyday life.