Wednesday, March 7, 2012
Star formation by collapse of molecular clouds
Simulation by SPH of the collapse and fragmentation of a molecular cloud presented in "The Formation of Stars
and Brown Dwarfs and the Truncation of Protoplanetary Discs in a Star Cluster" by Matthew R. Bate, Ian A. Bonnell, and Volker Bromm (http://www.ukaff.ac.uk/starcluster/).
Subscribe to:
Post Comments (Atom)
Featured Post
IBSE about Light Pollution
Here is my presentation that happened in the Discover the Cosmos Conference (Volos, Greece - 2013). The presentation was an Inquiry Base...
Twitter Updates
<- widget2 ->
Tweets by @eufisica
Popular Posts
-
In 1968, the crew of Apollo 8 became the first humans to witness and photograph the Earth appearing to rise over the horizon of the moo...
-
Nuclear Reactions In nuclear physics and nuclear chemistry , a nuclear reaction is semantically considered to be the process in which...
-
EN: A team of scientist made the most concise simulation about the collision of two neutron's stars. ES: Un equipo de científicos hi...
No comments:
Post a Comment