![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_10.jpg)
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
![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)
![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)