منابع مشابه
Clusters in the solar neighbourhood : how are they destroyed ?
We predict the survival time of initially bound star clusters in the solar neighbourhood taking into account: (1) stellar evolution, (2) tidal stripping, (3) shocking by spiral arms and (4) encounters with giant molecular clouds. We find that the predicted dissolution time is tdis = 1.7(Mi/10 4 M⊙) 0.67 Gyr for clusters in the mass range of 10 < Mi < 10 5 M⊙. The resulting predicted shape of th...
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We predict the survival time of initially bound star clusters in the solar neighbourhood taking into account: (1) stellar evolution, (2) tidal stripping, (3) shocking by spiral arms and (4) encounters with giant molecular clouds. We find that the predicted dissolution time is tdis = 1.7(Mi/10 4 M⊙) 0.67 Gyr for clusters in the mass range of 10 < Mi < 10 5 M⊙. The resulting predicted shape of th...
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ژورنال
عنوان ژورنال: The Journal of American History
سال: 1977
ISSN: 0021-8723
DOI: 10.2307/1888346