Add to ORKGThe observed relationship between mass-luminosity ratios for groups and clusters of galaxies and their population is interpreted on basis of a model developed by the author (1968) in which unstable groups of galaxies are thought to be the result of the fragmentation of a parent galaxy.Asociación Argentina de Astronomí
LaTex, 24 pages, 12 figuresWe have collected a large body of NIR (H band), UV (2000 A) and Halpha me...
We present results for a galaxy formation model that includes a simple treatment for the disruption ...
Evolutionary synthesis models for stellar populations of various ages and chemical compositions are ...
The observed relationship between mass-luminosity ratios for groups and clusters of galaxies and the...
hrough a convenient model, it is shown that galaxies with a condensed nuclear body breaking in two p...
Journal ArticleWe present a method capable of determining the evolutionary stage of bound, isolated...
Modeling of the velocity field of the Local Supercluster leads to the conclusion that there must be ...
I study the effect of the galaxies of the Milky Way subgroup on the chemical enrichment of the diffu...
Aims.We analyse the effects of a first generation of fast rotating massive stars on the dynamical a...
We analyze the three catalogs of nearby loose groups compiled by A. M. Garcia. She identified groups...
Since the appearance of the widely used model proposed by Press and Schechter (1974), much theoreti...
During an extensive program of direct imagery of emission nebulae, arcuate structures were found aro...
Galaxy morphologies in clusters have undergone a remarkable transition over the past several billion...
Gravitationally unstable, shocked layers of interstellar gas are produced by cloud-cloud collisions ...
We study the mass-to-light ratio of galaxy systems from poor groups to rich clusters and present for...
LaTex, 24 pages, 12 figuresWe have collected a large body of NIR (H band), UV (2000 A) and Halpha me...
We present results for a galaxy formation model that includes a simple treatment for the disruption ...
Evolutionary synthesis models for stellar populations of various ages and chemical compositions are ...
The observed relationship between mass-luminosity ratios for groups and clusters of galaxies and the...
hrough a convenient model, it is shown that galaxies with a condensed nuclear body breaking in two p...
Journal ArticleWe present a method capable of determining the evolutionary stage of bound, isolated...
Modeling of the velocity field of the Local Supercluster leads to the conclusion that there must be ...
I study the effect of the galaxies of the Milky Way subgroup on the chemical enrichment of the diffu...
Aims.We analyse the effects of a first generation of fast rotating massive stars on the dynamical a...
We analyze the three catalogs of nearby loose groups compiled by A. M. Garcia. She identified groups...
Since the appearance of the widely used model proposed by Press and Schechter (1974), much theoreti...
During an extensive program of direct imagery of emission nebulae, arcuate structures were found aro...
Galaxy morphologies in clusters have undergone a remarkable transition over the past several billion...
Gravitationally unstable, shocked layers of interstellar gas are produced by cloud-cloud collisions ...
We study the mass-to-light ratio of galaxy systems from poor groups to rich clusters and present for...
LaTex, 24 pages, 12 figuresWe have collected a large body of NIR (H band), UV (2000 A) and Halpha me...
We present results for a galaxy formation model that includes a simple treatment for the disruption ...
Evolutionary synthesis models for stellar populations of various ages and chemical compositions are ...