Relativistic Binaries in Globular Clusters
The galactic population of globular clusters are old, dense star systems, with a typical cluster containing $10^4 - 10^6$ stars. As an old population of stars, globular clusters contain many collapsed and degenerate objects. As a dense population of stars, globular clusters are the scene of many int...
Päätekijä: | |
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Aineistotyyppi: | Artikkeli |
Kieli: | English |
Julkaistu: |
SpringerOpen
2002-01-01
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Sarja: | Living Reviews in Relativity |
Aiheet: | |
Linkit: | http://www.livingreviews.org/lrr-2002-2 |