Supportive evidence for a brown dwarf solar companion

被引：0
|
作者：
Matese, JJ [1 ]
机构：
[1] Univ SW Louisiana, Lafayette, LA 70504 USA
来源：
PLANETARY SYSTEMS IN THE UNIVERSE OBSERVATION, FORMATION AND EVOLUTION | 2004年 / 202期
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中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We have previously given evidence based on Oort cloud comet orbital elements which suggested that there may be a Jovian-mass brown dwarf in our solar system. An extended cometary database is now available. The analyses have been repeated and we find that the set of statistically significant correlated anomalies is enhanced. We also respond to unsupported objections that have been raised to this conjecture. If real, the wide-binary object would constitute a natural dynamical intermediary between gas giant planetary objects and isolated objects.
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页码：214 / 216
页数：3
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