@article {292,
	title = {{Unveiling the radio counterparts of two binary AGN candidates: J1108+0659 and J1131-0204}},
	journal = {\aap},
	volume = {588},
	year = {2016},
	pages = {A102},
	keywords = {galaxies: active, galaxies: interactions, galaxies: nuclei, radio continuum: galaxies, techniques: interferometric},
	doi = {10.1051/0004-6361/201528021},
	author = {Bondi, M. and Perez-Torres, M.~A. and Piconcelli, E. and Fu, H.}
}
@article {2015ApJ...799...11X,
	title = {{ALMA Observations of Warm Dense Gas in NGC 1614 - Breaking of the Star Formation Law in the Central Kiloparsec}},
	journal = {The Astrophysical Journal},
	volume = {799},
	year = {2015},
	month = {jan},
	pages = {11},
	abstract = {We present ALMA Cycle-0 observations of the CO (6-5) line emission and of the 435 {$μ$}m dust continuum emission in the central kiloparsec of NGC 1614, a local luminous infrared galaxy at a distance of 67.8 Mpc (1$\{$$^{\prime \prime }$$\}$= 329 pc). The CO emission is well resolved by the ALMA beam (0.{\textquoteright}{\textquoteright}26 {\times} 0.{\textquoteright}{\textquoteright}20) into a circumnuclear ring, with an integrated flux of f $_{ CO(6-5)}$ = 898 ({\plusmn} 153) Jy km s$^{-1}$, which is 63({\plusmn} 12)\% of the total CO (6-5) flux measured by Herschel. The molecular ring, located between 100 pc {\l}t} r {\l}t} 350 pc from the nucleus, looks clumpy and includes seven unresolved (or marginally resolved) knots with median velocity dispersion of \~{}40 km s$^{-1}$. These knots are associated with strong star formation regions with {$Σ$}$_{SFR}$ \~{} 100 M $_{\&sun;}$ yr$^{-1}$ kpc$^{-2}$ and {$Σ$} $_{Gas}${\tilde} 10$^{4}$ $\{$M$\}$\_{\sun} pc$^{-2}$. The non-detections of the nucleus in both the CO (6-5) line emission and the 435 {$μ$}m continuum rule out, with relatively high confidence, a Compton-thick active galactic nucleus in NGC 1614. Comparisons with radio continuum emission show a strong deviation from an expected local correlation between {$Σ$}$_{Gas}$ and {$Σ$}$_{SFR}$, indicating a breakdown of the Kennicutt-Schmidt law on the linear scale of \~{}100 pc. The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc.},
	keywords = {galaxies: active, galaxies: evolution, galaxies: general, galaxies: interactions, galaxies: ISM, galaxies: magnetic fields, galaxies: nuclei, galaxies: starburst, submillimeter: galaxies},
	doi = {10.1088/0004-637X/799/1/11},
	url = {http://adsabs.harvard.edu/abs/2015ApJ...799...11X},
	author = {Xu, C.~K. and Cao, C. and Lu, N. and Gao, Y. and Diaz-Santos, T. and R. Herrero-Illana and Meijerink, R. and Privon, G. and Zhao, Y.-H. and Evans, A.~S. and K{\"o}nig, S. and Mazzarella, J.~M. and Aalto, S. and Appleton, P. and Armus, L. and Charmandaris, V. and Chu, J. and Haan, S. and Inami, H. and Murphy, E.~J. and Sanders, D.~B. and Schulz, B. and van der Werf, P.}
}
@article {231,
	title = {{Multiple AGN in the crowded field of the compact group SDSS J0959+1259}},
	journal = {MNRAS},
	volume = {453},
	year = {2015},
	pages = {214-221},
	keywords = {galaxies: active, galaxies: interactions, galaxies: Seyfert, X-rays: galaxies},
	doi = {10.1093/mnras/stv1623},
	url = {http://adsabs.harvard.edu/abs/2015MNRAS.453..214D},
	author = {De Rosa, A. and Bianchi, S. and Bogdanovi{\'c}, T. and Decarli, R. and Herrero-Illana, R. and Husemann, B. and Komossa, S. and Kun, E. and Loiseau, N. and Paragi, Z. and P{\'e}rez-Torres, M. and Piconcelli, E. and Schawinski, K. and Vignali, C.}
}
@article {2013MNRAS.434..978V,
	title = {{Molecular gas in type 2 quasars at z {\tilde} 0.2-0.3}},
	journal = {Monthly Notices of the Royal Astronomical Society},
	volume = {434},
	year = {2013},
	month = {sep},
	pages = {978-991},
	abstract = {{We present results of CO(1-0) spectroscopic observations of 10 Sloan Digital Sky Survey type 2 quasars (QSO2) at z {\tilde} 0.2-0.3 observed with the 30-m IRAM radio telescope and the Australia Telescope Compact Array. We report five new confirmed CO(1-0) detections and one tentative detection. They have L\^{}{\textquoteright} $\}$\_CO {\tilde} several {\times} 10$^{9}$ K km s$^{-1}$ pc$^{2}$, while upper limits for the non-detections are L\^{}{\textquoteright} $\},
	keywords = {galaxies: evolution, galaxies: interactions, quasars: general},
	author = {Villar-Mart{\'\i}n, M. and M. Rodr{\'\i}guez and Drouart, G. and Emonts, B. and Colina, L. and Humphrey, A. and S. Garc{\'\i}a-Burillo and Graci{\'a} Carpio, J. and Planesas, P. and P{\'e}rez Torres, M. and Arribas, S.}
}
@article {2013MNRAS.435.2335B,
	title = {{The NGC 3341 minor merger: a panchromatic view of the active galactic nucleus in a dwarf companion}},
	journal = {Monthly Notices of the Royal Astronomical Society},
	volume = {435},
	year = {2013},
	month = {nov},
	pages = {2335-2344},
	abstract = {We present X-ray (Chandra), radio (Expanded Very Large Array and European VLBI Network) and archival optical data of the triple-merging system in NGC 3341. Our panchromatic analysis confirms the presence of a Seyfert 2 active galactic nucleus (AGN) in NGC 3341B, one of the secondary dwarf companions. On the other hand, the nucleus of the primary galaxy, consistent with a star-forming region of a few solar masses per year, and NGC 3341C are very unlikely to host an AGN. We therefore suggest that NGC 3341 is an exceptional example of an AGN triggered in the satellite galaxy of a minor-merging system. The existence of such a system can have important implications in the models of hierarchical growth of structures. Further observational and theoretical efforts on NGC 3341 and potentially similar sources are needed in order to understand the role of minor mergers on the onset of AGN activity, and in the evolution of massive galaxies.},
	keywords = {galaxies: active, galaxies: interactions, galaxies: Seyfert, X-rays: individual: NGC 3341},
	doi = {10.1093/mnras/stt1459},
	url = {http://adsabs.harvard.edu/abs/2013MNRAS.435.2335B},
	author = {Bianchi, S. and Piconcelli, E. and M. A. P{\'e}rez-Torres and Fiore, F. and La Franca, F. and Mathur, S. and Matt, G.}
}
@article {190,
	title = {{SDSS J002531.46-104022.2 at z = 0.30: a candidate for the (ultra)luminous infrared galaxy to optical quasar transition}},
	journal = {MNRAS},
	volume = {432},
	year = {2013},
	pages = {2104-2111},
	keywords = {galaxies: evolution, galaxies: interactions, quasars: individual: SDSS J002531.46-104022.2},
	doi = {10.1093/mnras/stt538},
	url = {http://adsabs.harvard.edu/abs/2013MNRAS.432.2104V},
	author = {Villar-Mart{\'\i}n, M. and Emonts, B. and M. Rodr{\'\i}guez and Torres, M.~P. and Drouart, G.}
}
