Collision tomography: the progenitor of the Andromeda stellar stream and the metallicity gradient

Details Collision tomography: the progenitor of the Andromeda stellar stream and the metallicity gradient Collision tomography: the progenitor of the Andromeda stellar stream and the metallicity gradient

Aug 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1269..400m&link_type=abstract

THE 10TH INTERNATIONAL SYMPOSIUM ON ORIGIN OF MATTER AND EVOLUTION OF GALAXIES: OMEG-2010. AIP Conference Proceedings, Volume 1

Computer Science

Galaxies, Accretion, Artificial Satellites, Dwarf Galaxies, Infall, Accretion, And Accretion Disks, Artificial Earth Satellites

Scientific paper

Using N-body simulations of the interaction between an accreting
satellite and M31, we have successfully reproduced observed distribution
of the Andromeda stellar stream. We predict the spatial distribution of
the metal in the progenitor dwarf galaxy by the comparison with the
recent observations and the simulations.

Affiliated with

Also associated with

No associations

Rating

Collision tomography: the progenitor of the Andromeda stellar stream and the metallicity gradient does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Collision tomography: the progenitor of the Andromeda stellar stream and the metallicity gradient, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Collision tomography: the progenitor of the Andromeda stellar stream and the metallicity gradient will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1862724