scholarly journals Small and very small interstellar grains

2000 ◽  
Vol 105 (A5) ◽  
pp. 10299-10302 ◽  
Author(s):  
A. N. Witt
Keyword(s):  
Nature ◽  
1970 ◽  
Vol 225 (5235) ◽  
pp. 834-836 ◽  
Author(s):  
S. NARANAN ◽  
G. A. SHAH
Keyword(s):  
X Rays ◽  

2004 ◽  
Vol 429 (2) ◽  
pp. 371-381 ◽  
Author(s):  
N. V. Voshchinnikov ◽  
V. B. Il'in ◽  
Th. Henning

Nature ◽  
1965 ◽  
Vol 205 (4966) ◽  
pp. 59-60 ◽  
Author(s):  
M. J. BAINES ◽  
I. P. WILLIAMS
Keyword(s):  

1971 ◽  
Vol 12 (1) ◽  
pp. 250-255 ◽  
Author(s):  
G. A. Shah ◽  
M. S. Vardya

1991 ◽  
Vol 126 ◽  
pp. 349-356
Author(s):  
Mark R. Showalter

AbstractEach of the outer gas giants Jupiter, Saturn, Uranus and Neptune is now known to be encircled by a system of rings. Some of these, such as the A, B, and C rings of Saturn and the nine narrow Uranian rings, are rather optically thick and are composed primarily of large bodies (1 cm to 10 m). However, every other system has been found to contain a large population of micron-sized dust. Such rings reveal the effects of a variety of physical processes that are also acting on interplanetary and interstellar grains. When such rings are examined as members of a general class, recurring patterns begin to emerge.


Author(s):  
A. P. Jones ◽  
A. G. G. M. Tielens ◽  
D. J. Hollenbach ◽  
C. F. McKee
Keyword(s):  

Sign in / Sign up

Export Citation Format

Share Document