![SOLVED: 1. Jeans collapse In this problem you will derive the Jeans mass, discussed in lecture: (Scharf: equation 2.16; Perryman: just after equation 10.1). Calculate the gravitational potential energy of a uniform SOLVED: 1. Jeans collapse In this problem you will derive the Jeans mass, discussed in lecture: (Scharf: equation 2.16; Perryman: just after equation 10.1). Calculate the gravitational potential energy of a uniform](https://cdn.numerade.com/ask_images/48f3094dec57459588fd830db71d2b57.jpg)
SOLVED: 1. Jeans collapse In this problem you will derive the Jeans mass, discussed in lecture: (Scharf: equation 2.16; Perryman: just after equation 10.1). Calculate the gravitational potential energy of a uniform
![Formation of proto-clusters and star formation within clusters: apparent universality of the initial mass function? | Astronomy & Astrophysics (A&A) Formation of proto-clusters and star formation within clusters: apparent universality of the initial mass function? | Astronomy & Astrophysics (A&A)](https://www.aanda.org/articles/aa/full_html/2012/09/aa19440-12/aa19440-12-eq191.png)
Formation of proto-clusters and star formation within clusters: apparent universality of the initial mass function? | Astronomy & Astrophysics (A&A)
A diagram that shows the Jeans mass as a function of number density for... | Download Scientific Diagram
![Lecture 6: Jeans mass & length Anisotropies in the CMB temperature density ripples at the time of decoupling. These are the seeds that grow to form galaxies. - ppt download Lecture 6: Jeans mass & length Anisotropies in the CMB temperature density ripples at the time of decoupling. These are the seeds that grow to form galaxies. - ppt download](https://images.slideplayer.com/32/10033996/slides/slide_4.jpg)