:. Projects
:. Asteroseismology
:. Dark Matter Galaxies
:. EPR
:. Gravitophotons
:. Hybrid Rocket Engine
:. Pulse-Ram Induction

:. Sections:
:. Primer

:. Presentation:
:. Slide 01
:. Slide 02
:. Slide 03
:. Slide 04
:. Slide 05
:. Slide 06
:. Slide 07
:. Slide 08
:. Slide 09
:. Slide 10
:. Slide 11
:. Slide 12
:. Slide 13
:. Slide 14
:. Slide 15
:. Slide 16
:. Slide 17
:. Slide 18
:. Slide 19

:. Feedback:
:. thegraben@gmail.com

:. Sponsors
:. The Graben: Dark Matter Galaxies Presentation .:

A proto galactic cloud of material starts to collapse. Initially the halo components are formed like in normal galaxies, but as time goes on the collapse slows for unknown reasons. So, what we are left with is a low density galaxy, which might contain a small number of stars, but would be hard to observe.