Binaries as Tracers Stellar Ev
Book Details
Format
Hardback or Cased Book
ISBN-10
0521433584
ISBN-13
9780521433587
Publisher
Cambridge University Press
Imprint
Cambridge University Press
Country of Manufacture
GB
Country of Publication
GB
Publication Date
Nov 26th, 1992
Print length
304 Pages
Weight
679 grams
Dimensions
25.40 x 17.90 x 1.80 cms
Product Classification:
Galaxies & starsGalaxies and starsAstrophysics
Ksh 24,650.00
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Binary stars are considered as one of the best constraints on stellar formation models. Observations on multiple stellar systems are discussed in these proceedings, first published in 1992, with the aim of disentangling evidence of stellar formation from later physical evolution.
More than two-thirds of stars belong to multiple stellar systems. Binary stars are considered now as one of the best constraints on stellar formation models. Not only do binaries keep memory of their birth conditions but their orbit will also be subjected to changes by tidal effects, wind accretion and encounters in clusters. Certainly the correlation between orbital eccentricity and period is a clue to our understanding of double star history. These proceedings aim to disentangle evidence of stellar formation from later physical evolution. Each article in this 1992 volume is a paper that was read at a meeting organized to honour Dr Roger Griffin of the University of Cambridge for his pioneer work in galactic astronomy, dynamics of clusters and study on binary stars due to his cross-correlation technique to determine stellar radial velocities.
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