HI in Nearby Dwarf Galaxies: Comparing Simulations and Observations

Details HI in Nearby Dwarf Galaxies: Comparing Simulations and Observations HI in Nearby Dwarf Galaxies: Comparing Simulations and Observations

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21531804j&link_type=abstract

American Astronomical Society, AAS Meeting #215, #318.04; Bulletin of the American Astronomical Society, Vol. 42, p.319

Mathematics

Logic

Scientific paper

What fuels continued star formation in the Milky Way disk remains an
open question. We test the hypothesis that dwarf galaxies bring gas to
the Milky Way disk by comparing state-of-the-art cosmological
simulations of a disk galaxy and high-resolution HI observations.

Affiliated with

Also associated with

No associations

Rating

HI in Nearby Dwarf Galaxies: Comparing Simulations and Observations 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 HI in Nearby Dwarf Galaxies: Comparing Simulations and Observations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and HI in Nearby Dwarf Galaxies: Comparing Simulations and Observations will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-961815