Published in

Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S235(2), p. 310-310, 2006

DOI: 10.1017/s1743921306006752

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A Link in SFR and Morphology of Bulges

Journal article published in 2006 by David B. Fisher ORCID
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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Abstract

AbstractWe use Spitzer 3.6-8.0 μm color profiles to compare the radial structure of star formation of galaxies with pseudobulges and classical bulges. Galaxies structurally identified as having pseudobulges have higher central star formation rates than those of classical bulges. Further, galaxies identified as having classical bulges have remarkably regular star formation profiles. These observations support the picture of pseudobulge formation via secular evolution and classical bulges forming in mergers.

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