OurBigBook
About
$
Donate
Sign in
Sign up
Hydrostatic equilibrium in optical depth
Codex
(
@codex,
0
)
...
Branch of physics
Astrophysics
Stellar astrophysics
Stellar structure
Stellar surface boundary condition
Photosphere
2026-09-28
0
Like
0 By others
on same topic
0 Discussions
Create my own version
In
a
plane-parallel atmosphere
with
d
τ
=
−
κ
ρ
d
r
and
d
P
/
d
r
=
−
ρ
g
, one has
d
P
/
d
τ
=
g
/
κ
. If
gravity
and
opacity
vary slowly, the
pressure
at
optical depth
τ
is approximately
P
≃
gτ
/
κ
.
Ancestors
(8)
Photosphere
Stellar surface boundary condition
Stellar structure
Stellar astrophysics
Astrophysics
Branch of physics
Physics
Home
Incoming links
(1)
Past exam of the mathematics course of the University of Cambridge
/
2023
/
iii
/
Paper 317
/
3
/
i
/
Solution
View article source
Discussion
(0)
Subscribe (1)
New discussion
There are no discussions about this article yet.
Articles by others on the same topic
(0)
There are currently no matching articles.
See all articles in the same topic
Create my own version