Initial mass function problem

In summary, the conversation discusses finding the constant a for a newly formed globular cluster with a total mass of 10^6 times the mass of the sun and an initial mass function of dN/dm = a.m^-2.35 in the mass range of 0.1 - 20 times the mass of the sun. The number of stars in a globular cluster is estimated to be between 10^4 - 10^6, but the equation should yield a smaller value. The solution involves performing an integration, which the person asking the question was able to successfully do with the help of the person responding.
  • #1
kranav
34
0

Homework Statement



the question says, consider a newly formed globular cluster, with a total mass 10^6 times mass of the sun and an initial mass function dN/dm = a.m^-2.35 in the mass range 0.1 - 20 times mass of the sun, where m = M/mass of the sun.
find the constant a. (answer : 1.9 x10^5)
thanks.

Homework Equations





The Attempt at a Solution



the number of stars in a globular cluster are between 10^4 - 10^6. but N from the above equation should be smaller as the mass range is from 0.1 to 20 times sun's mass. If I can find that N the equation is a piece of cake.
 
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  • #3
I'm really sorry about that ... wasn't aware of that. I thought if I could reframe the question and start afresh
 
  • #4
After looking up "initial mass function", it looks like the number of stars in the mass range [itex]m_0[/itex] to [itex]m_1[/itex] is given by

[tex]N=\int_{m_0}^{m_1}\frac{dN}{dm}mdm[/tex]

Have you tried performing this integration?
 
  • #5
Yes this time I got it. Thank you very much
 

1. What is the Initial Mass Function (IMF) problem?

The Initial Mass Function problem refers to the challenge of understanding and predicting the distribution of stellar masses in a given star-forming region. It is concerned with determining the number of stars that are formed at different masses and the reasons behind this distribution.

2. Why is the IMF problem important in astrophysics?

The IMF problem is important because it helps us understand the formation and evolution of stars and galaxies. The distribution of stellar masses has a significant impact on the chemical and dynamical processes in galaxies, and therefore, understanding the IMF is crucial for understanding the structure and evolution of the universe.

3. What are some proposed solutions to the IMF problem?

There are several proposed solutions to the IMF problem, including top-down and bottom-up approaches. Top-down approaches involve analyzing the properties of a large sample of stars in a particular star-forming region to determine the IMF, while bottom-up approaches involve modeling the physical processes involved in star formation to predict the IMF.

4. What challenges do scientists face in studying the IMF problem?

One of the main challenges in studying the IMF problem is the limited observational data available, especially for low-mass stars. This makes it difficult to accurately determine the IMF in different star-forming regions. Additionally, the physical processes involved in star formation are complex and not fully understood, making it challenging to develop accurate models.

5. What are the potential implications of solving the IMF problem?

Solving the IMF problem could have significant implications for our understanding of the universe. It could help us better understand the formation and evolution of galaxies, improve our predictions of stellar populations, and aid in the search for habitable planets and potential extraterrestrial life. It could also have implications for other areas of astrophysics, such as dark matter and cosmology.

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