Starbursts, Metallicity, and the Disruption of Dwarf Galaxies

Astronomy and Astrophysics – Astronomy

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Scientific paper

Major starburst events can last tens of millions of years, and in the process they can deposit significant amounts of energy into the surrounding interstellar medium. This energy from supernovae and stellar winds imparts enough momentum to the interstellar medium that portions of the ISM can become unbound and leave the parent galaxy, taking the metal enriched stellar debris along. In dwarf galaxies, starbursts can produce enough total energy to unbind most or all of the ambient ISM. Whether this actually occurs is a strong function of the ellipticity of the ISM distribution, with flat disks and spheres being the limiting cases. We calculate whether "blow out" along the symmetry axis or "blow away" of the entire ISM occurs in dwarf galaxies as a function of galactic mass, starburst energy, ISM density and ISM ellipticity. We find that for physically reasonable values of these parameters a blow out along the symmetry axis occurs in the majority of cases, though a significant fraction of small dwarf galaxies can lose most of their ISM. The effects of this range of behavior on the metallicities that would be observed in these galaxies is examined.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Starbursts, Metallicity, and the Disruption of Dwarf Galaxies 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 Starbursts, Metallicity, and the Disruption of Dwarf Galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Starbursts, Metallicity, and the Disruption of Dwarf Galaxies will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-781448

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.