A PHYSICAL MODEL FOR THE IRAS ZODIACAL DUST BANDS

被引：12

作者：

JONES, MH ^{[1
]}

ROWANROBINSON, M ^{[1
]}

机构：

[1] QUEEN MARY & WESTFIELD COLL, SCH MATH SCI, ASTRON UNIT, LONDON E1 4NS, ENGLAND

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1993年 / 264卷 / 01期

关键词：

INTERPLANETARY MEDIUM; SOLAR SYSTEM; GENERAL; INFRARED;

D O I：

10.1093/mnras/264.1.237

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present a model, based on justifiable physical assumptions, of the zodiacal cloud and asteroidal dust bands which gives a good representation of the thermal IR emission from interplanetary dust observed using IRAS. In addition to the narrow asteroidal bands that have been previously reported, we find a broad double-band component with peak intensities at beta almost-equal-to +/- 9-degrees, which shows significant emission at latitudes \beta\ approximately 20-degrees. The physical significance of this feature within the Solar system and its relationship to the zodiacal cloud are discussed.

引用

页码：237 / 247

页数：11

共 50 条

[21] ORIGINS OF ZODIACAL DUST CLOUD
HARWIT, M
JOURNAL OF GEOPHYSICAL RESEARCH, 1963, 68 (08): : 2171 - +
[22] The structured zodiacal light: IRAS, COBE, and ISO observations
Reach, WT
DIFFUSE INFRARED RADIATION AND THE IRTS, 1997, 124 : 33 - 40
[23] THE GLOBAL DISTRIBUTION OF ZODIACAL DUST
KNEISSEL, B
IAU SYMPOSIA, 1990, (139): : 231 - 232
[24] Physical properties of asteroid dust bands and their sources
Nesvorny, D
Vokrouhlicky, D
Bottke, WF
Sykes, M
ICARUS, 2006, 181 (01) : 107 - 144
[25] The contribution of asteroid dust to the interplanetary dust cloud: The impact of ULYSSES results on the understanding of dust production in the asteroid belt and of the formation of the IRAS dust bands
Mann, I
Grun, E
Wilck, M
ICARUS, 1996, 120 (02) : 399 - 407
[26] Dust masses and star formation in bright IRAS galaxies - Application of a physical model for the interpretation of FIR observations
Misiriotis, A
Papadakis, IE
Kylafis, ND
Papamastorakis, J
ASTRONOMY & ASTROPHYSICS, 2004, 417 (01) : 39 - 50
[27] An improved model for the infrared emission from the zodiacal dust cloud: cometary, asteroidal and interstellar dust
Rowan-Robinson, M.
May, B.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2013, 429 (04) : 2894 - 2902
[28] New measurements of the motion of the zodiacal dust
Reynolds, RJ
Madsen, GJ
Moseley, SH
ASTROPHYSICAL JOURNAL, 2004, 612 (02): : 1206 - 1213
[29] Temporal variation of the zodiacal dust cloud
Napier, WM
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2001, 321 (03) : 463 - 470
[30] ON LOCATION IN SPACE OF ZODIACAL DUST PARTICLES
WOLSTENCROFT, RD
PLANETARY AND SPACE SCIENCE, 1967, 15 (06) : 1081 - +

← 1 2 3 4 5 →