The ejection velocity of meteoroids from cometary nuclei deduced from observations of meteor shower outbursts

被引：10

作者：

Ma, YH ^{[1
]}

Williams, IP

机构：

[1] Acad Sinica, Purple Mt Observ, Nanjing 210008, Peoples R China

[2] Acad Sinica, Natl Astron Observ, Beijing, Peoples R China

[3] Univ London Queen Mary & Westfield Coll, Astron Unit, London E1 4NS, England

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2001年 / 325卷 / 01期

关键词：

comets : individual : 55P/Tempel -Tuttle; comets : individual : 109P/SwiftTuttle; meteors; meteoroids;

D O I：

10.1046/j.1365-8711.2001.04440.x

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The ejection velocities of meteoroids belonging to the Leonid and Perseid meteoroid streams are deduced from the observed differences between the longitude of the ascending node of the outburst meteoroids and that of the parent comet. The difference is very sensitive to the true anomaly of the ejection point, as well as the ejection velocity, and probable values for both are discussed.

引用

页码：379 / 384

页数：6

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