Compact group galaxies are a common phase in galaxy evolution and provide insight into the process that transforms galaxies from isolated, star forming late-type galaxies to passive galaxies in high density environments. I mapped spectrally the central and middle regions of 40 galaxies in 10 Southern Compact Groups and established group membership by redshift. Of the eight groups with all members observed, I found that one galaxy is not in the group in four cases. I obtained ages and metallicities of the stellar populations using the STARLIGHT code to summarize past star formation and current activity. Galaxies that are part of a group showed both high-metallicity stellar populations, indicating rapid processing of gas through multiple star...
We present the results of a study comparing the stellar populations in the elliptical galaxies of Hi...
Context.Multi-wavelength observations of Hickson's Compact Groups (HCGs) have shown that many of the...
Using local properties of galaxies can help us to further understand the process of internal galaxy ...
Aims. We study the star formation fistory (SFH) of 210 galaxy members of 55 Hickson compact groups ...
We present an in depth study on the evolution of galaxy properties in compact groups over the past 3...
We present a multi-wavelength analysis of three compact galaxy groups, Hickson compact groups (HCGs)...
Compact groups provide an environment to study the growth of galaxies amid multiple prolonged intera...
If we are to develop a comprehensive and predictive theory of galaxy formation and evolution, it is ...
Aims. This paper is part of a series in which we systematically compare the properties of galaxies i...
We present an analysis of the spectra of 62 galaxies in 15 compact groups. The galaxies are classifi...
Abstract This paper reviews recent observations of the history of star formation in galaxies, and th...
Across cosmic time, stars have contributed most of the radiant energy found in the Universe and have...
Galaxies in the local Universe are characterized by blue, star-forming disk galaxies, and red, massi...
Compact groups of galaxies provide insight into the role of low-mass, dense environments in galaxy e...
The first stars formed in the early universe and shortly after assembled into the first galaxies. Si...
We present the results of a study comparing the stellar populations in the elliptical galaxies of Hi...
Context.Multi-wavelength observations of Hickson's Compact Groups (HCGs) have shown that many of the...
Using local properties of galaxies can help us to further understand the process of internal galaxy ...
Aims. We study the star formation fistory (SFH) of 210 galaxy members of 55 Hickson compact groups ...
We present an in depth study on the evolution of galaxy properties in compact groups over the past 3...
We present a multi-wavelength analysis of three compact galaxy groups, Hickson compact groups (HCGs)...
Compact groups provide an environment to study the growth of galaxies amid multiple prolonged intera...
If we are to develop a comprehensive and predictive theory of galaxy formation and evolution, it is ...
Aims. This paper is part of a series in which we systematically compare the properties of galaxies i...
We present an analysis of the spectra of 62 galaxies in 15 compact groups. The galaxies are classifi...
Abstract This paper reviews recent observations of the history of star formation in galaxies, and th...
Across cosmic time, stars have contributed most of the radiant energy found in the Universe and have...
Galaxies in the local Universe are characterized by blue, star-forming disk galaxies, and red, massi...
Compact groups of galaxies provide insight into the role of low-mass, dense environments in galaxy e...
The first stars formed in the early universe and shortly after assembled into the first galaxies. Si...
We present the results of a study comparing the stellar populations in the elliptical galaxies of Hi...
Context.Multi-wavelength observations of Hickson's Compact Groups (HCGs) have shown that many of the...
Using local properties of galaxies can help us to further understand the process of internal galaxy ...