Autor: |
Keshet, Uri, Hopman, Clovis, Alexander, Tal |
Rok vydání: |
2009 |
Předmět: |
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Zdroj: |
Astrophys.J.698:L64-L67,2009 |
Druh dokumentu: |
Working Paper |
DOI: |
10.1088/0004-637X/698/1/L64 |
Popis: |
We analyze the distribution of stars of arbitrary mass function xi(m) around a massive black hole (MBH). Unless xi is strongly dominated by light stars, the steady-state distribution function approaches a power-law in specific energy x=-E/(m*sigma^2)Comment: Revised version published in Astrophys. J. Lett |
Databáze: |
arXiv |
Externí odkaz: |
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