Elementary Astronomy - Initial Mass Function

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SUMMARY

The discussion focuses on estimating the number of low (0.5 Solar Mass) and high (50 Solar Mass) stars in the Milky Way Galaxy using the Initial Mass Function (IMF) defined by the equation \(\xi = \xi_0 M^{-2.3}\). The Star Formation Rate is approximately 1 Solar Mass per year, predominantly forming 0.5 Solar Mass stars. The lifetime of stars is described by \(L = \frac{10^{10} \text{y}}{M^{2.5}}\). The constant \(\xi_0\) can be determined from the condition \(\xi = 2\) when \(M = 0.5\), allowing for further calculations of star distribution.

PREREQUISITES
  • Understanding of the Initial Mass Function (IMF)
  • Familiarity with stellar lifetimes and mass relationships
  • Basic knowledge of astronomical units and measurements
  • Ability to manipulate algebraic equations
NEXT STEPS
  • Research the derivation and implications of the Initial Mass Function (IMF)
  • Study the relationship between stellar mass and lifespan using \(L = \frac{10^{10} \text{y}}{M^{2.5}}\)
  • Explore methods for estimating star formation rates in galaxies
  • Investigate the role of \(\xi_0\) in stellar population synthesis
USEFUL FOR

Astronomy students, astrophysicists, and researchers interested in stellar population dynamics and the evolution of galaxies.

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Homework Statement


Estimate the number of low and high mass stars that you expect to find in our Milky Way Galaxy now. Use the following (very approximate but about right numbers) for your estimate:

The Star Formation Rate in our galaxy is approximately 1 Solar Mass per year and virtually all of this goes into making =~ 0.5 Solar Mass stars. The Initial Mass Function, Xi, describes the number of stars at each mass and is something like:

\xi = \xi0 M-2.3

where M is the mass of the stars in Solar Masses. In lecture it was shown that the lifetime of stars is given by

L = 1010y / M2.5

If the galaxy is 10 billion years old, how many 0.5 and 50 Solar Mass stars do you expect to find in the galaxy.

Homework Equations



\xi = \xi0 M-2.3
L = 1010y / M2.5

The Attempt at a Solution



My attempt lies around trying to understand exactly what \xi0 is. Although we haven't learned it in class, I know that the IMF is meant to describe a distribution of initial solar masses in stars in the galaxy. Obviously, in this case we're not meant to do it in the standard fashion.

I note that when \xi0 is 1 then
\xi = 5 @ M = 0.5 and
\xi = 0.02 @ M = 50

Which tells me that the function is working to some extent but without some explanation as to what \xi0 is I can barely comprehend what I am meant to do with this question. I hope I'm not missing something completely obvious, but this question is confusing.
 
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Update:

I consulted my professor as I was handing in this assignment (Without this question completed) And he explained to me that \xi0 is a constant, that can be determined from \xi = 2 when M = 0.5. And from there the rest of the variables can be determined.
 
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