Bulge Formation Patterns in APM-SPH simulations: Questions to Be Answered by Future Missions

Details Bulge Formation Patterns in APM-SPH simulations: Questions to Be Answered by Future Missions Bulge Formation Patterns in APM-SPH simulations: Questions to Be Answered by Future Missions

Dec 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011sf2a.conf..157o&link_type=abstract

SF2A-2011: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics Eds.: G. Alecian, K. Belkacem,

Astronomy and Astrophysics

Astrophysics

Theory, Galaxies, Bulges, Structure, Kinematics, Abundances

Scientific paper

The few observations of bulges available suggest a bi-modality in their properties, feature we have also found in high resolution hydrodynamical simulations in a cosmological context. The latter gives important information about bulge formation processes, facilitating the comparison with available observational data, as well as serving as guideline for future observational strategies. We conclude that in this particular field, there is much need for more in depth observations of large samples in order to distinguish among the variety of possible bulge formations paths.

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