Bulges of Nearby Galaxies-What Are the Structures We See in the Centers of Disk Galaxies?

Details Bulges of Nearby Galaxies-What Are the Structures We See in the Centers of Disk Galaxies? Bulges of Nearby Galaxies-What Are the Structures We See in the Centers of Disk Galaxies?

Jun 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1240..195d&link_type=abstract

HUNTING FOR THE DARK: THE HIDDEN SIDE OF GALAXY FORMATION. Edited by Victor P. Debattista and Cristina C. Popescu AIP Conferen

Computer Science

Galaxies, Star Formation, Brightness, Stellar Mass, Spiral Galaxies, Star Formation, Magnitudes And Colors, Luminosities, Masses

Scientific paper

Using bulge-disk decompositions of light profiles in combined HST plus ground-based imaging in the V-band and also in near-IR HST-NICMOS plus Spitzer 3.6 μm data, we are investigating the structural properties of bulges and their correlations with bulge morphology and kinematics in galaxies of Hubble type Sa-Scd. Additionally, Spitzer observations at 8 μm and 24 μm reveal star formation activity in disks and their bulges and its correlation with disk and bulge properties.

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