437 citations
- D. Hughes5 profiles23 · h 66
- I. Aretxaga3 profiles17 · h 49
- A. Bressan2 profiles16 · h 70
- E. Terlevich16 · h 38
- D. Scott4 profiles15 · h 114
- M. Halpern2 profiles13 · h 85
- G. Tenorio-Tagle12 · h 35
- M. Plionis2 profiles12 · h 33
- R. Terlevich2 profiles12 · h 49
- E. Chapin11 · h 43
- G. Granato2 profiles11 · h 45
- S. Silich2 profiles11 · h 21
- Cardiff UniversityGB17 papers
- Instituto de Astrofísica de CanariasES17 papers
- Osservatorio Astronomico di PadovaIT17 papers
- Universidad Nacional Autónoma de MéxicoMX17 papers
- University of British ColumbiaCA17 papers
- California Institute of TechnologyUS15 papers
- Scuola Internazionale Superiore di Studi AvanzatiIT13 papers
- Durham UniversityGB12 papers
- Jet Propulsion LaboratoryUS12 papers
- National Observatory of AthensGR11 papers
- Royal ObservatoryGB11 papers
- University of EdinburghGB11 papers
135 papers
Spectroscopic monitoring of the Blazar 3C 454.3
E. Benitez, V. H. Chavushyan, C. M. Raiteri +5
We performed an optical spectroscopic monitoring of the blazar 3C 454.3 from September 2003 to July 2008. Sixteen optical spectra were obtained during different runs, which constit…
Age and Extinction of the Ultraviolet Emitting Regions in M82
L. H. Rodriguez-Merino, D. Rosa-Gonzalez, Y. D. Mayya +3
The M82 galaxy has been the subject of several studies basically because it is relatively close to to the Milky Way and it displays a strong star formation activity. Using multi-ba…
M82 as a Galaxy: Morphology and Stellar Content of the Disk and Halo
Y. Divakara Mayya, Luis Carrasco
For decades, the nuclear starburst has taken all the limelight in M82 with very little discussion on M82 as a galaxy. The situation is changing over the last decade, with the publi…
Over half of the far-infrared background light comes from galaxies at z >= 1.2
Mark J. Devlin, Peter A. R. Ade, Itziar Aretxaga +26
Submillimetre surveys during the past decade have discovered a population of luminous, high-redshift, dusty starburst galaxies. In the redshift range 1 <= z <= 4, these massive sub…
On the Heating Efficiency Derived from Observations of Young Super Star Clusters in M82
Sergiy Silich, Guillermo Tenorio-Tagle, Ana Torres Campos +2
Here we discuss the mechanical feedback that massive stellar clusters provide to the interstellar medium of their host galaxy. We apply an analytic theory developed in a previous s…
The 3D velocity structure of the planetary nebula NGC 7009
W. Steffen, M. Espindola, S. Martinez +1
In search for deviations from homologous expansion in planetary nebulae we present a 3D morphokinematical model of NGC 7009. The model has been constructed with {\em Shape} based o…