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Stars and Star Clusters / Sterne und Sternhaufen (Landolt-Bornstein Numerical Data and Functional Relationships in Science and Technology) by L.H. Aller

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Published by Springer .
Written in English


  • Astrophysics,
  • Mathematics and Science,
  • Astronomy - General,
  • Science,
  • Science/Mathematics,
  • Magnetism,
  • Physics,
  • Science / Physics,
  • Stars,
  • Stern,
  • Sternhaufen,
  • Astrophysics & Space Science

Book details:

The Physical Object
Number of Pages456
ID Numbers
Open LibraryOL9054073M
ISBN 103540109765
ISBN 109783540109761

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A much-needed book for amateurs, as there is little info out there on star clusters (there are some graduate-level textbooks, but not even many of these). The information is rather disjointed and the pictures could be improved. Many typos hopefully all will be improved in a 2nd by: Abstract. Star clusters, studied for three centuries, have in the last decade assumed ever-increasing importance for several reasons. The emphasis on the two types of stellar populations puts them in the spotlight since galactic clusters represent population I and globular clusters population II. Stars are born in turbulent molecular clouds that fragment and collapse under the influence of their own gravity, forming a cluster of hundred or more stars. The star formation process is controlled by the interplay between supersonic turbulence and gravity. In this work, the properties of stellar clusters created by numerical simu-. Sterne werden nicht isoliert sondern in Gruppen, bekannt als Sternhaufen ge-boren. Sternhaufen sind beobachtet worden in einer Vielzahl von Galaxien Die Analyse der Sternhaufen, ihrer Masse, ihres Alters und ihrer Ausdehnung Star clusters lying in these galaxies were observed through HST imaging and VLT spectroscopy. The analysis of.

Kupte knihu Stars and Star Clusters / Sterne und Sternhaufen (L.H. Aller, I. Appenzeller, B. Baschek, H.W. Duerbeck) za Kč v ověřeném obchodě. Prolistujte stránky knihy, přečtěte si recenze čtenářů, nechte si doporučit podobnou knihu z nabídky více než 19 miliónů titulů. Stars and Star Clusters / Sterne und Sternhaufen Prisoner of the Sultan Wallace & Gromit Post-Keynesian Economics Mazda Motorsports The Psychology of Adolescent Satanism The Day Vegan Challenge (Updated Edition) Developing Wind Power Projects Managing Information Security Risk Captain Superlative City Maps Baghdad Iraq Parks, Plants, and People. Ein Sternhaufen ist eine Gruppe von Sternen, die einen gemeinsamen Ursprung haben und durch die Schwerkraft für eine gewisse Zeit zusammengehalten werden. Da angenommen wird, dass Sternhaufen Sterne ähnlichen Alters und ähnlicher Zusammensetzung enthalten, haben Forscher sie als "astronomisches Laboratorium" benutzt, um zu verstehen, wie die. Ihsan Hafez, Francis Richard Stephenson & Wayne Orchiston, “The Investigation of Stars, Star Clusters and Nebulae in ‘Abd al-Raḥmān al-Ṣūfī’s Book of the Fixed Stars”, in: W. Orchiston, D.A. Green & R.G. Strom (eds.), New Insights From Recent Studies in Historical Astronomy: Following the Footsteps of F. Richard Stephenson.

(Redirected from Index Catalogue of Nebulae and Clusters of Stars) The New General Catalogue of Nebulae and Clusters of Stars (abbreviated NGC) is an astronomical catalogue of deep-sky objects compiled by John Louis Emil Dreyer in The NGC contains 7, objects, including galaxies, star clusters, emission nebulae and absorption nebulae. grouped way, in the basic unit of a star cluster, so that both the mass function of stars formed within a star cluster and the mass function of star clusters in a galaxy need to be known for a quantitative description of galaxy-wide star formation. Stars and star clusters: Sterne und Sternhaufen, allemand: Untersuchungen über die absoluten Helligkeiten und die räumliche Verteilung der F-Sterne: Zahlenwerte und Funktionen aus Naturwissenschaften und Technik. This thesis examines the properties of extended star clusters and ultra-compact dwarf galaxies (UCDs), and aims to establish their nature and provide insights into their formation mechanisms. In terms of their sizes and magnitudes, they are both located in the gap region between classical dwarf galaxies and globular clusters (GCs), which challenged many previous definitions of what constitutes.