With the main goal of finding bulgeless galaxies harbouring supermassive black holes and showing, at most, just residual star formation activity,we have selected a sample ofmassive bulgeless red sequence galaxies from the Sloan Digital Sky Survey - Data Release 7 (SDSS DR7), based on the NewYork UniversityValue-Added Galaxy Catalogue. Multiwavelength data were retrieved using European Virtual Observatory (EURO-VO) tools, and the objects are characterized in terms of degree of star formation and the presence of an AGN.We have found seven objects that are quenched massive galaxies, have no prominent bulge and showsigns of extra activity in their nuclei, five of them being central in their halo. These objects are rather robust candidates for rare systems that, though devoid of a significant bulge, harbour a supermassive black hole with an activity level likely capable of having halted the star formation through feedback. © 2013 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society.
CITATION STYLE
Coelho, B., Antón, S., Lobo, C., & Ribeiro, B. (2013). Red bulgeless galaxies in SDSS DR7. Are there any AGN hosts? Monthly Notices of the Royal Astronomical Society, 436(3), 2426–2434. https://doi.org/10.1093/mnras/stt1736
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