This article reviews the popular reasons for the belief that dwarf elliptical galaxies and (ordinary) elliptical galaxies are distinct and separate species. They include: light-profile shape (or similarly image concentration); the magnitude-central surface brightness diagram; the magnitude-effective surface brightness diagram (or similarly the magnitude-effective radius diagram); and the Fundamental Plane. It is shown how a continuous trend between luminosity and a) light-profile shape, and b) central surface brightness (until the onest of core formation at MB ∼ -20.5 mag), results in a unification of the dwarf elliptical and (ordinary) elliptical galaxies. Neither the above four reasons, nor the luminosity function (at least in the Virgo c...
The structural properties of elliptical galaxies are consistent with their formation in a merging hi...
Context. Dwarf elliptical galaxies (dEs) are the most abundant in the Universe. Research into these ...
Low surface brightness dwarf galaxies (at least the gas-poor variety) represent a fundamentally dist...
Dwarf elliptical galaxies are frequently excluded from bright galaxy samples because they do not fol...
Aims. The present work is aimed at studying the distribution of galaxies of different types and lum...
We present preliminary results of an extensive study of the fundamental properties of dwarf elliptic...
New surface photometry of all known elliptical galaxies in the Virgo cluster is combined with publis...
We present preliminary results of an extensive study of the fundamental properties of dwarf elliptic...
This paper is the first in a series in which we present the results of an ESO Large Program on the k...
This paper is the first in a series in which we present the results of an ESO Large Program on the k...
We review the systematic properties of ``dwarf'' elliptical (dE) galaxies, focussing on the relation...
The dwarf elliptical galaxies (dEs) are more luminous than dwarf spheroidals and fainter than “norma...
Galaxies can be classified in two broad sequences which are likely to reflect their formation mechan...
This paper is the first in a series in which we present the results of an ESO Large Program on the k...
none7We report on a complete CCD imaging survey of 226 elliptical galaxies in the North-East quadran...
The structural properties of elliptical galaxies are consistent with their formation in a merging hi...
Context. Dwarf elliptical galaxies (dEs) are the most abundant in the Universe. Research into these ...
Low surface brightness dwarf galaxies (at least the gas-poor variety) represent a fundamentally dist...
Dwarf elliptical galaxies are frequently excluded from bright galaxy samples because they do not fol...
Aims. The present work is aimed at studying the distribution of galaxies of different types and lum...
We present preliminary results of an extensive study of the fundamental properties of dwarf elliptic...
New surface photometry of all known elliptical galaxies in the Virgo cluster is combined with publis...
We present preliminary results of an extensive study of the fundamental properties of dwarf elliptic...
This paper is the first in a series in which we present the results of an ESO Large Program on the k...
This paper is the first in a series in which we present the results of an ESO Large Program on the k...
We review the systematic properties of ``dwarf'' elliptical (dE) galaxies, focussing on the relation...
The dwarf elliptical galaxies (dEs) are more luminous than dwarf spheroidals and fainter than “norma...
Galaxies can be classified in two broad sequences which are likely to reflect their formation mechan...
This paper is the first in a series in which we present the results of an ESO Large Program on the k...
none7We report on a complete CCD imaging survey of 226 elliptical galaxies in the North-East quadran...
The structural properties of elliptical galaxies are consistent with their formation in a merging hi...
Context. Dwarf elliptical galaxies (dEs) are the most abundant in the Universe. Research into these ...
Low surface brightness dwarf galaxies (at least the gas-poor variety) represent a fundamentally dist...