Optical Extinction Help Needed: Calculating A_v for Spherical Cloud

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SUMMARY

The discussion focuses on calculating the maximum optical extinction, A_{v}, for a spherical cloud with a mass of 1 M(sun) and a diameter of 1 parsec. The radial density of the cloud follows a power law described by ρ(r) ∝ r^{−α}. Participants reference the equation N(H) = 6.93 × 10^{21} cm^{-2} × A_{v}/R_{v} with R_{v} set to 3, indicating a specific approach to determining column density and extinction values.

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  • Understanding of optical extinction and its significance in astrophysics
  • Familiarity with power law density functions
  • Knowledge of column density calculations
  • Basic grasp of spherical geometry in astrophysical contexts
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  • Explore the application of power law density profiles in astrophysics
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Ayame17
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Help Needed! Optical extinction

Homework Statement



Spherical cloud (gas to dust ratio 100) with mass = 1 M(sun), diameter = 1pc. Radial density can be described by power law (see below). Determine the maximum optical extinction, ie. the function A_{v}(\alpha).

Homework Equations



Power law: \rho(r) \propto r^{-\alpha}

You may use N(H)=6.93*10^{21} cm^{-2}*A_{v}/R_{v} and R_{v}=3

The Attempt at a Solution



I've looked up column density and found extinction values calculated by flux, but simply can't see where to even begin. A nudge in the right direction would be so very helpful!
 
Last edited:
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Please, anyone?
 

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