The Structure of the Underlying Stellar Host in Blue Compact Dwarf Galaxies

Details The Structure of the Underlying Stellar Host in Blue Compact Dwarf Galaxies The Structure of the Underlying Stellar Host in Blue Compact Dwarf Galaxies

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005rmxac..24..223c&link_type=abstract

II International GTC Workshop: Science with GTC 1st-light Instruments and the LMT (Eds. A. M. Hidalgo-Gámez, J. J. González, J.

Astronomy and Astrophysics

Astronomy

Galaxies: Evolution, Galaxies: Star Formation

Scientific paper

Nowadays it is well established that BCDs are mostly old systems, as the vast majority of them have an extended low-surface brightness (LSB) stellar host underlying their central starburst component. This host generally extends several kpc from the star-forming (SF) regions, shows regular elliptical isophotes, and displays red colors indicative of an evolved stellar population Papaderos96a,Cairos01a,Cairos01b,Cairos03.

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