A possible source of the X-rays from Comet Hyakutake

被引：30

作者：

Northrop, TG ^{[1
]}

Lisse, CM ^{[1
]}

Mumma, MJ ^{[1
]}

Desch, MD ^{[1
]}

机构：

[1] UNIV MARYLAND,DEPT ASTRON,COLLEGE PK,MD 20742

来源：

ICARUS | 1997年 / 127卷 / 01期

关键词：

D O I：

10.1006/icar.1997.5694

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The soft X rays from Comet Hyakutake observed by Lisse et al, (1996, Science 274, 205-209) can reasonably be attributed to electron-neutral and electron-dust collisions, The neutrals and dust come from the comet and the electrons from the solar wind and from photoionization of neutrals, We assume the electron energy spectrum shape to be the same as seen by Vega 2 at Halley's comet, but otherwise use cometary and solar wind parameters observed at Hyakutake.

引用

页码：246 / 250

页数：5

共 14 条

[11]

MCDONNELL JAM, 1991, COMETS POST HALLEY E, V2, P1043

[12] A COMETARY AURORA [J].