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

Bibcode
2005RMxAC..24..223C
Caon, N.; Cairós, L. M.; Aguerri, J. A. L.; Muñoz-Tuñon, C.; Papaderos, P.; Noeske, K.
Bibliographical reference

II International GTC Workshop: Science with GTC 1st-light Instruments and the LMT (Eds. A. M. Hidalgo-Gámez, J. J. González, J. M. Rodríguez Espinosa, and S. Torres-Peimbert) Revista Mexicana de Astronomía y Astrofísica (Serie de Conferencias) Vol. 24, pp. 223-224 (2005) (http://www.astroscu.unam.mx/~rmaa/)

Advertised on:
12
2005
Number of authors
6
IAC number of authors
1
Citations
2
Refereed citations
2
Description
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.
Type
Non-refereed
Galaxies
Star formation

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