ISOCAM observations of the Comet P/Kopff dust trail

被引：20

作者：

Davies, JK

Sykes, MV

Reach, WT

Boulanger, F

Sibille, F

Cesarsky, CJ

机构：

[1] STEWARD OBSERV,TUCSON,AZ

[2] UNIV PARIS 11,INST ASTROPHYS SPATIALE,ORSAY,FRANCE

[3] OBSERV LYON,LYON,FRANCE

[4] CEA SACLAY,SERV ASTROPHYS,F-91191 GIF SUR YVETTE,FRANCE

来源：

ICARUS | 1997年 / 127卷 / 01期

基金：

美国国家航空航天局;

关键词：

D O I：

10.1006/icar.1997.5684

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present the results of two scans through the dust trail of Comet P/Kopff made with ISOCAM on 26 March 1996. Positions behind the comet at mean anomalies of 0.5 degrees and 1 degrees less than the nucleus were imaged using the LW10 (IRAS Band 1, 12 mu m) filter. The trail is clearly detected and appears to have varied since it was observed with the IRAS satellite in 1983. (C) 1997 Academic Press.

引用

页码：251 / 254

页数：4

共 6 条

[1]

Cesarsky CJ, 1996, ASTRON ASTROPHYS, V315, pL32

[2]

Kessler MF, 1996, ASTRON ASTROPHYS, V315, pL27

[3]

Stewart B. C., 1984, Journal of the British Interplanetary Society, V37, P348

[4]

Sykes M.V., 1986, ADV SPACE RES, V6, P67

[5] THE DISCOVERY OF DUST TRAILS IN THE ORBITS OF PERIODIC COMETS [J].

SYKES, MV ;

LEBOFSKY, LA ;

HUNTEN, DM ;

LOW, F .

SCIENCE, 1986, 232 (4754) :1115-1117

[6] COMETARY DUST TRAILS .1. SURVEY [J].

SYKES, MV ;

WALKER, RG .

ICARUS, 1992, 95 (02) :180-210

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