Add to ORKGThe M81 group consists of a few large galaxies and about 40 dwarf galaxies. It is a highly interacting group which makes it an important nearby laboratory to study the role of the environment and interactions in the dwarf galaxy formation and evolution. We use the resolved stellar populations in a sample of early-type dwarf galaxies in this group to derive the photometric metallicity distribution functions and study the potential presence of population gradients in this dwarf galaxy sample
Aims. We focus on the resolved stellar populations of one early-type and four transition-type dwarf ...
We present surface photometry and metallicity measurements for 104 nearby dwarf galaxies imaged with...
Aims. We explore correlations between the strength of metallicity gradients in Local Group dwarf gal...
The M81 group is a highly interacting group consisting of a few large galaxies and about 40 dwarfs o...
We study the properties of the dwarf galaxy population in the nearby interacting M81 group of galaxi...
Aims. We study the dwarf spheroidal galaxies in the nearby M 81 group in order to construct their ph...
Aims. We study the dwarf spheroidal galaxies in the nearby M 81 group in order to construct their p...
The study of (dwarf) galaxies in nearby groups is one among the most powerful tools that can be used...
This thesis presents results from two projects using photometric observations to investigate stellar...
Aims. We focus on the resolved stellar populations of one early-type and four transition-type dwarf ...
The dwarf elliptical galaxies (dEs) are more luminous than dwarf spheroidals and fainter than “norma...
Aims. We focus on the resolved stellar populations of one early-type and four transition-type dwarf ...
Aims. We study dwarf galaxies in the Centaurus A group to investigate their metallicity and possible...
Aims. We study dwarf galaxies in the Centaurus A group to investigate their metallicity and possible...
Aims. We investigate the present-day photometric properties of the dwarf spheroidal galaxies in the ...
Aims. We focus on the resolved stellar populations of one early-type and four transition-type dwarf ...
We present surface photometry and metallicity measurements for 104 nearby dwarf galaxies imaged with...
Aims. We explore correlations between the strength of metallicity gradients in Local Group dwarf gal...
The M81 group is a highly interacting group consisting of a few large galaxies and about 40 dwarfs o...
We study the properties of the dwarf galaxy population in the nearby interacting M81 group of galaxi...
Aims. We study the dwarf spheroidal galaxies in the nearby M 81 group in order to construct their ph...
Aims. We study the dwarf spheroidal galaxies in the nearby M 81 group in order to construct their p...
The study of (dwarf) galaxies in nearby groups is one among the most powerful tools that can be used...
This thesis presents results from two projects using photometric observations to investigate stellar...
Aims. We focus on the resolved stellar populations of one early-type and four transition-type dwarf ...
The dwarf elliptical galaxies (dEs) are more luminous than dwarf spheroidals and fainter than “norma...
Aims. We focus on the resolved stellar populations of one early-type and four transition-type dwarf ...
Aims. We study dwarf galaxies in the Centaurus A group to investigate their metallicity and possible...
Aims. We study dwarf galaxies in the Centaurus A group to investigate their metallicity and possible...
Aims. We investigate the present-day photometric properties of the dwarf spheroidal galaxies in the ...
Aims. We focus on the resolved stellar populations of one early-type and four transition-type dwarf ...
We present surface photometry and metallicity measurements for 104 nearby dwarf galaxies imaged with...
Aims. We explore correlations between the strength of metallicity gradients in Local Group dwarf gal...