Tidal Tales of Minor Mergers: Star Formation in the Tidal Debris of Minor Mergers

Astronomy and Astrophysics – Astrophysics – Cosmology and Extragalactic Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

4 pages. To appear in the proceedings of "Galaxy Wars: Stellar Populations and Star Formation in Interacting Galaxies" (Tennes

Scientific paper

How does the tidal debris of minor galaxy mergers contribute to structures in spiral galaxies or in the intergalactic medium? While major mergers are known to create structures such as tidal dwarf galaxies and star clusters within their tidal debris, less is known about minor mergers (mass ratios between a dwarf galaxy and disk galaxy of less than one-third) and their tidal debris. This work surveys 6 nearby minor mergers using optical broad-band and H-alpha narrow-band imaging to characterize star formation in their tidal debris. Young star clusters with ages less than the dynamical age of the tidal tails are found in all 6 mergers, indicating that the star clusters formed in situ. Even if minor mergers contribute less tidal debris per interaction than major mergers, they are more common and possibly contribute structure to all types of galaxies and to the intergalactic medium throughout the history of the universe.

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

Tidal Tales of Minor Mergers: Star Formation in the Tidal Debris of Minor Mergers 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 Tidal Tales of Minor Mergers: Star Formation in the Tidal Debris of Minor Mergers, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Tidal Tales of Minor Mergers: Star Formation in the Tidal Debris of Minor Mergers will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-427669

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