Full text: The internal constitution of the stars

RADIATIVE EQUILIBRIUM 
113 
v' radiation corresponds to the temperature drop in 2 cm. The net outward 
flow for v' is thus only one-hundredth of that of v". 
If v' represents 1 per cent, of the radiation and v" the remaining 99 per 
cent., the absorption-line at v' will double the total amount of absorption 
and emission going on; although constituting but a small part of the 
radiation it does as much business as all the rest put together. This means 
that Jc t is doubled. But as regards opacity the effect is that 1 per cent, of 
the radiation suffers an almost complete check, and the rest flows through 
as before. Hence & 2 is only increased 1 per cent.
	        
Waiting...

Note to user

Dear user,

In response to current developments in the web technology used by the Goobi viewer, the software no longer supports your browser.

Please use one of the following browsers to display this page correctly.

Thank you.