AGN Feedback and Quenching of Star Formation: A Multiwavelength Approach with the EURO-VO

被引：1
|
作者：
Coelho, B. [1 ,2 ]
Lobo, C. [1 ,2 ]
Anton, S. [3 ,4 ]
机构：
[1] Univ Porto, Ctr Astrofis, Rua Estrelas, P-4150762 Oporto, Portugal
[2] Univ Porto, Fac Ciencias, P-4169007 Oporto, Portugal
[3] Univ Porto, Fac Ciencias, CICGE, P-4169007 Oporto, Portugal
[4] Univ Lisbon, Fac Ciencias, SIM, P-1649016 Lisbon, Portugal
来源：
ENVIRONMENT AND THE FORMATION OF GALAXIES: 30 YEARS LATER: PROCEEDINGS OF SYMPOSIUM 2 OF JENAM 2010 | 2011年
关键词：
DIGITAL SKY SURVEY; GALAXIES;
D O I：
10.1007/978-3-642-20285-8_19
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
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.
引用
收藏
页码：99 / +
页数：2
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