Jesús Jiménez Fuensalida
Current Organizations / Institutes
The organizations/institutes from the scholar's latest article
Research Subjects
Research Interests
Jesús Jiménez Fuensalida has a total of 21 co-authors. Here are the top co-authors by number of shared publications:
- Abdelmajid Benhida1 shared publication
- Ana Maria Pérez Garcia
ISDEFE for European Space Astronomy Centre (ESAC)/ESA
1 shared publication - Antonia M. Varela
Instituto de Astrofísica de Canarias, 38205-La Laguna, Tenerife, Spain
1 shared publication - Casiana Munoz-Tunon
Instituto de Astrofísica de Canarias cmt
1 shared publication - Diego García Lambas
Grupo de Investigaciones en Astronomía Teórica y Experimental (IATE) Universidad Nacional de Córdoba Observatorio Astronómico Laprida 854 5000 Córdoba Argentina
1 shared publication - Gianluca Lombardi
European Southern Observatory Santiago 19 19001 Casilla Chile
1 shared publication
Latest Publications
- 1 November 2011
- Published by IOP Publishing in Publications of the Astronomical Society of the Pacific
- Vol. 123 (909) , 1334-1346
European Extremely Large Telescope Site Characterization I: Overview
- 1 November 2011
- Published by IOP Publishing in Publications of the Astronomical Society of the Pacific
- Vol. 123 (909) , 1334-1346
European Extremely Large Telescope Site Characterization I: Overview
- Open Access
- 1 February 2000
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 529 (2) , 875-885
Far‐InfraredISOMaps of Active Galaxies
Far-IR Infrared Space Observatory (ISO) maps of four Seyfert galaxies are presented and compared with their optical counterpart images. The far-IR maps resemble the optical images of these galaxies when degraded to the ISO resolution. The spatial extension of the far-IR maps is also comparable to the optical extension of these objects, an indication of the extended nature of their far-IR emission. The 90 μm intensity profiles of these galaxies show that there is a disk component noticeable in the far IR. NGC 3079 shows a 90 μm halo extending far out of the galaxy plane. NGC 4051 shows a dark molecular cloud whose far-IR output could be as large as that of the active nucleus itself, demonstrating that very bright IR sources other than the active nucleus may be responsible for a large fraction of the far-IR emission in some Seyfert galaxies.
- 1 February 2000
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 529 (2) , 875-885
Open AccessFar‐InfraredISOMaps of Active Galaxies
Far-IR Infrared Space Observatory (ISO) maps of four Seyfert galaxies are presented and compared with their optical counterpart images. The far-IR maps resemble the optical images of these galaxies when degraded to the ISO resolution. The spatial extension of the far-IR maps is also comparable to the optical extension of these objects, an indication of the extended nature of their far-IR emission. The 90 μm intensity profiles of these galaxies show that there is a disk component noticeable in the far IR. NGC 3079 shows a 90 μm halo extending far out of the galaxy plane. NGC 4051 shows a dark molecular cloud whose far-IR output could be as large as that of the active nucleus itself, demonstrating that very bright IR sources other than the active nucleus may be responsible for a large fraction of the far-IR emission in some Seyfert galaxies.