Physical Processes in Gaseous Nebulae. VIII. The Ultraviolet Radiation Field and Electron Temperature of an Optically Thick Nebula.

1939 ◽  
Vol 90 ◽  
pp. 601 ◽  
Author(s):  
Lawrence H. Aller ◽  
James G. Baker ◽  
Donald H. Menzel
2000 ◽  
Vol 197 ◽  
pp. 403-413
Author(s):  
Doug Johnstone

The most likely processes responsible for the removal of circumstellar disks around young stars are reviewed with emphasis on the physical state of the disk during the period of destruction and the timescale for disk removal. Four disk dispersal mechanisms are discussed in detail: 1) viscous accretion of material onto the central source, 2) close stellar encounters, 3) stellar winds, and 4) photoevaporation by ultraviolet radiation. While viscous accretion is shown to be efficient in the inner regions of disks (r < 10 AU), photoevaporation is the principal process of disk dispersal at large radii (r > 10 AU). The commonly held view that stellar winds removed the remnant Solar Nebula is seriously questioned.


1987 ◽  
Vol 315 ◽  
pp. 180 ◽  
Author(s):  
Jill Bechtold ◽  
Ray J. Weymann ◽  
Zuo Lin ◽  
Matthew A. Malkan

2000 ◽  
Vol 21 (1-2) ◽  
pp. 19-27 ◽  
Author(s):  
Archana Samantaray ◽  
Pushpa Khare

1938 ◽  
Vol 88 ◽  
pp. 422 ◽  
Author(s):  
James G. Baker ◽  
Donald H. Menzel ◽  
Lawrence H. Aller.

1941 ◽  
Vol 93 ◽  
pp. 236 ◽  
Author(s):  
Lawrence H. Aller

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