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19972012
most citedThe starburst-AGN connection in the merger galaxy Mrk 938: an infrared and X-ray view

18 citations · 18 across the 1 of their papers we have counts for

collaborators

8 papers

astro-ph.CO2012★ 18 cited

The starburst-AGN connection in the merger galaxy Mrk 938: an infrared and X-ray view

P. Esquej, A. Alonso-Herrero, A. M. Pérez-García +14

Mrk938 is a luminous infrared galaxy in the local Universe believed to be the remnant of a galaxy merger. It shows a Seyfert 2 nucleus and intense star formation according to optic…

astro-ph2006

Flat-spectrum symmetric objects with ~1 kpc sizes I. The candidates

Pedro Augusto, J. Ignacio Gonzalez-Serrano, Ismael Perez-Fournon +1

In order to understand the origin and evolution of radio galaxies, searches for the youngest such sources have been conducted. Compact-medium symmetric objects (CSO-MSOs) are thoug…

astro-ph1997

Red quasars not so dusty

C. R. Benn, M. Vigotti, R. Carballo +2

Webster et al (1995) claimed that up to 80% of QSOs may be obscured by dust. They inferred the presence of this dust from the remarkably broad range of B-K optical-infrared colours…

astro-ph1997

Observations of the Hubble Deep Field with the Infrared Space Observatory. IV. Association of sources with Hubble Deep Field Galaxies

The ISO-HDF Consortium, :, Bob Mann

We discuss the identification of sources detected by ISO at 6.7 and 15 micron in the Hubble Deep Field (HDF) region. We conservatively associate ISO sources with objects in existin…

astro-ph1997

Observations of the Hubble Deep Field with the Infrared Space Observatory. V. Spectral Energy Distributions, Starburst Models and Star Formation History

The ISO-HDF Consortium, :, Michael Rowan-Robinson

We have modelled the spectral energy distributions of the 13 HDF galaxies reliably detected by ISO. For 2 galaxies the emission detected by ISO is consistent with being starlight o…

astro-ph1997

Observations of the Hubble Deep Field with the Infrared Space Observatory. III. Source counts and P(D) analysis

The ISO-HDF Consortium, :, Seb Oliver

We present source counts at 6.7 micron and 15 micron from our maps of the Hubble Deep Field region, reaching 38.6 microJy at 6.7 micron and 255 microJy at 15 micron. These are the…