The evolution of an SNR in a high-density medium has been studied using analytical and numerical hydrodynamic and photoionization models. The models show that...
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PublicaciónThe starburst model for active galactic nuclei - The broad-line region as supernova remnants evolving in a high-density medium
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PublicaciónThe starburst model for active galactic nuclei-II. The nature of the lag
In the starburst model for active galactic nuclei (AGN), the observed broad emission lines and their variability are generated by compact, strongly radiative...
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PublicaciónThe Starburst-Active Galactic Nucleus Connection in Active Galaxies: The MassiveNuclear Star-Forming Disk in NGC 4303
Two-dimensional spectroscopy of the low-redshift active galaxy NGC 4303 obtained with the Two-Dimensional Fiber ISIS System is presented. The ionization...
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PublicaciónThe starburst-active galactic nucleus connection in the merger galaxy Mrk 938: an infrared and X-ray view
Mrk 938 is a luminous infrared (IR) galaxy in the local Universe believed to be the remnant of a galaxy merger. It shows a Seyfert 2 nucleus and intense star...
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PublicaciónThe State-of-Play of Anomalous Microwave Emission (AME) research
Anomalous Microwave Emission (AME) is a component of diffuse Galactic radiation observed at frequencies in the range ≈ 10-60 GHz. AME was first detected in 1996...
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PublicaciónThe statistics of voids as a tool to constrain cosmological parameters: σ8 and Γ
We present a general analytical formalism to calculate accurately several statistics related to underdense regions in the Universe. The statistics are computed...
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PublicaciónThe Stellar and Gaseous Kinematics in NGC 253
This paper presents observations made at intermediate spectral and spatial resolutions along the major and minor axes of the starburst galaxy NGC 253. The...
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PublicaciónThe Stellar Atmosphere Physical System I. Phenomenological Definition and Representation of a Stellar Atmosphere
This paper is the first in a series of two that deals with the physical and numerical grounds of stellar atmospheres modelling. After a phenomenological...
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PublicaciónThe Stellar Atmosphere Physical System II. An Operative Sequential Algorithm to Solve the Stellar Atmosphere Problem
In this paper, the second and the last of the series, we present a sequential algorithm to solve the stellar atmosphere problem that may serve as a paradigm for...