Abstract
We selected bulgeless red sequence galaxies in the SDSS (DR7) [Abazajian et al., ApJS 182, 543 (2009)] using data from NYU-VAGC [Blanton et al., AJ 129, 2562 (2005)]. Using EURO-VO tools we obtained multiwavelength data, we built spectral energy distributions, and undertook a thorough analysis to ascertain: the frequency of AGN among these galaxies, the degree of star formation and intrinsic extinction. We aim at verifying whether there are bulgeless quenched galaxies hosting SMBHs in order to test the AGN feedback paradigm.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
References
K.N. Abazajian et al., ApJS 182, 543 (2009)
M.R. Blanton et al., AJ 129, 2562 (2005)
G. Kauffmann et al., MNRAS 346, 1055 (2003)
L. Kewley et al., ApJ 556, 121 (2001)
K. Schawinski et al., MNRAS 382, 1415 (2007)
G. Stasińska et al., MNRAS 371, 972 (2006)
Author information
Authors and Affiliations
Corresponding author
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 2011 Springer-Verlag Berlin Heidelberg
About this paper
Cite this paper
Coelho, B., Lobo, C., Antón, S. (2011). AGN Feedback and Quenching of Star Formation: A Multiwavelength Approach with the EURO-VO. In: Ferreras, I., Pasquali, A. (eds) Environment and the Formation of Galaxies: 30 years later. Astrophysics and Space Science Proceedings. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-20285-8_19
Download citation
DOI: https://doi.org/10.1007/978-3-642-20285-8_19
Published:
Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-642-20284-1
Online ISBN: 978-3-642-20285-8
eBook Packages: Physics and AstronomyPhysics and Astronomy (R0)