Temperature Effects of a Doubled Radiation Emission from an HII Region

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SUMMARY

The discussion centers on the effects of doubled radiation emission from an HII region on temperature dynamics. It concludes that increased radiation from the ionizing star raises the temperature due to the excess energy of ionizing photons, which translates into kinetic energy for the electron gas. The balance between heating from ionization and cooling from recombination processes establishes a local thermodynamic equilibrium, where the radius of the Strömgren sphere does not influence temperature determination. Calculating the average energy of photo-ejected electrons and the equilibrium temperature is essential for understanding the relationship between radiation increase and Strömgren sphere radius.

PREREQUISITES
  • Understanding of HII regions and Strömgren spheres
  • Knowledge of ionization processes and photon energy
  • Familiarity with thermodynamic equilibrium concepts
  • Basic principles of recombination and cooling mechanisms in astrophysics
NEXT STEPS
  • Explore the calculations for average energy of photo-ejected electrons in ionized gases
  • Research the relationship between ionization rates and recombination rates in HII regions
  • Study the impact of radiation pressure on the dynamics of HII regions
  • Investigate the role of temperature in determining the size of Strömgren spheres
USEFUL FOR

Astronomers, astrophysicists, and students studying stellar evolution and ionized gas dynamics will benefit from this discussion.

Poppop
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If the star ionizing an HII region suddenly doubled the radiation emitted, would that increase or decrease the temperature? I feel like the expansion of the region would cancel out the increased energy, but I don't know.
 
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My impression is that the temperature does indeed increase. I think that the growth in radius of a Strömgren sphere due to increase in radiation of the star is not an "expansion" of the sphere, but an shift of the limit at which the properties of the gas change. Taking this into account I would proceed as follows to make some calculations.

For most of the ionizing stars, a high fraction of the ionizing photons will have energies greater than the ionization energy of hydrogen. The excess of energy of the ionizing photons will become kinetic energy of the electron gas. Knowing the temperature of the star and considering this excess of energy, you should be able to calculate or make some assumption about the average energy of a photo-ejected electron.

On the other hand, the heating mechanisms will be balanced by cooling and the gas will tend to local thermodynamic equilibrium. I guess that cooling of the electron gas will be mainly due to recombination. You should be able to express the average energy that is loss in the gas for a single recombined electron. Probably there are other cooling processes, but this would make things too complex.

Since in equilibrium the recombination rate is equal to the ionization rate in the sphere, the energetic balance between those two quantities for an average electron should provide the equilibrium temperature. As you see, at least according to my understanding, the radius of the sphere does not have any impact on the determination of the temperature.

Knowing the temperature, the recombination rate \beta is known which provides the necessary information to calculate the radius of the Strömgren sphere. Putting things together you should come to an relation between the radius and the increase in radiation. This would be a nice exercise.
 
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