activity
20012013
most citedThe Expanding Nebular Remnant of the Recurrent Nova RS Ophiuchi (2006): II. Modeling of Combined Hubble Space Telescope Imaging and Ground-based Spectroscopy

58 citations · 156 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.CO2013★ 3 cited

What do the Star Formation Histories of Galaxies tell us about the Starburst-AGN connection?

J. P. Torres-Papaqui, R. Coziol, I. Plauchu-Frayn +2

Using a sample of 229618 narrow emission-line galaxies, we have determined the normal star formation histories (SFHs) for galaxies with different activity types: star forming galax…

astro-ph.CO2012★ 26 cited

The star formation histories of Hickson compact group galaxies

I. Plauchu-Frayn, A. del Olmo, R. Coziol +1

ABRIDGED: We study the Star Formation History (SFH) of 210 galaxies members of 55 Hickson Compact Groups (HCG) and 309 galaxies from the Catalog of Isolated Galaxies (CIG). The SFH…

astro-ph.CO2012★ 19 cited

The star formation history and chemical evolution of star forming galaxies in the nearby universe

J. P. Torres-Papaqui, R. Coziol, R. A. Ortega-Minakata +1

We have determined the O/H and N/O of a sample of 122751 SFGs from the DR7 of the SDSS. For all these galaxies we have also determined their morphology and their SFH using the code…

astro-ph.CO2012

What makes a galaxy radio-loud?

R. A. Ortega-Minakata, J. P. Torres-Papaqui, H. Andernach +5

We compare the Spectral Energy Distribution (SED) of radio-loud and radio-quiet AGNs in three different samples observed with SDSS: radio-loud AGNs (RLAGNs), Low Luminosity AGNs (L…

astro-ph.CO2011★ 6 cited

Mass of the black hole in the Seyfert 1.5 galaxy H 0507+164 from reverberation mapping

C. S. Stalin, S. Jeyakumar, R. Coziol +2

We present the results of our optical monitoring campaign of the X-ray source H 0507+164, a low luminosity Seyfert 1.5 galaxy at a redshift z = 0.018. Spectroscopic observations we…

astro-ph.GA2010

The signature of LLAGNs in the nearby universe

D. M. Neri-Larios, J. P. Torres-Papaqui, R. Coziol +2

We have used the diagnostic diagram that compares the ratio of emission lines [NII]\lambda6584/Hαwith the equivalent width of [NII]6584, as proposed by Coziol et al. (1998), to…