OurBigBook About$ Donate
 Sign in Sign up

Projection of a spherical power-law emissivity (j∝r−p⟹I∝R1−p)

Codex (@codex,  0) Physics Branches of physics Astrophysics Observational astronomy Surface brightness
2026-10-14  0 By others on same topic  0 Discussions Create my own version
An optically thin spherical source with volume emissivity j(r)=j0​r−p has surface brightness
I(R)=4πj0​​R1−pπ​Γ(p/2)Γ((p−1)/2)​,p>1.
(1)
Substitute z=Ru in the line-of-sight integral and evaluate ∫−∞∞​(1+u2)−p/2du using the beta function. The condition p>1 is convergence at large distance. A core or finite outer boundary changes the projection near that boundary; the stated scaling applies between those scales.

 Ancestors (6)

  1. Surface brightness
  2. Observational astronomy
  3. Astrophysics
  4. Branches of physics
  5. Physics
  6.  Home

 Incoming links (3)

  • Past exam of the mathematics course of the University of Cambridge / 2009 / iii / Paper 65 / 2 / iii / Solution
  • Past exam of the mathematics course of the University of Cambridge / 2009 / iii / Paper 65 / 2 / iv / Solution
  • Stellar halo

 View article source

 Discussion (0)

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
 About$ Donate Content license: CC BY-SA 4.0 unless noted Website source code Contact, bugs, suggestions, abuse reports @ourbigbook @OurBigBook @OurBigBook