Global properties of elliptical galaxies, such as the luminosity, radius, projected velocity dispersion, projected luminosity density, etc., form a two-dimensional family. This “fundamental plane” of elliptical galaxies can be defined by the velocity dispersion and mean surface brightness, and its thickness is presently given by the measurement error-bars only. This is indicative of a strong regularity in the process of galaxy formation. However, all morphological parameters which describe the shape of the distribution of light, and reflect dynamical anisotropics of stars, are completely independent from each other, and independent of the fundamental plane. The M/L ratios show only a small intrinsic scatter in a luminosity range spanning so...
VizieR online Data Catalogue associated with article published in journal Astronomical Journal (AAS)...
The disks of spiral galaxies are generally elliptical rather than circular. The distribution of elli...
Bright elliptical galaxies have a markedly different distribution of Hubble types than faint ellipti...
Global properties of elliptical galaxies, such as the luminosity, radius, projected velocity dispers...
The global properties of elliptical galaxies, such as luminosity, radius, projected velocity dispers...
In the poster as presented at the meeting, I described global morphological properties of elliptical...
The global properties of elliptical galaxies are connected through the so-called fundamental plane o...
We analyze the fundamental plane projections of elliptical galaxies as a function of luminosity, usi...
The global properties of elliptical galaxies are connected through the so-called fundamental plane ...
The structural properties of elliptical galaxies are consistent with their formation in a merging hi...
International audienceDensity profiles (NFW and similar) of structures found in cosmological LambdaC...
We present a new relation between velocity dispersion, surface brightness, and radius (or luminosity...
New surface photometry of all known elliptical galaxies in the Virgo cluster is combined with publis...
This paper reviews surface photometry of bulges and elliptical galaxies. Work prior to 1982 is discu...
Recent results from gravitational lensing are combined with new modeling of the stellar velocity dis...
VizieR online Data Catalogue associated with article published in journal Astronomical Journal (AAS)...
The disks of spiral galaxies are generally elliptical rather than circular. The distribution of elli...
Bright elliptical galaxies have a markedly different distribution of Hubble types than faint ellipti...
Global properties of elliptical galaxies, such as the luminosity, radius, projected velocity dispers...
The global properties of elliptical galaxies, such as luminosity, radius, projected velocity dispers...
In the poster as presented at the meeting, I described global morphological properties of elliptical...
The global properties of elliptical galaxies are connected through the so-called fundamental plane o...
We analyze the fundamental plane projections of elliptical galaxies as a function of luminosity, usi...
The global properties of elliptical galaxies are connected through the so-called fundamental plane ...
The structural properties of elliptical galaxies are consistent with their formation in a merging hi...
International audienceDensity profiles (NFW and similar) of structures found in cosmological LambdaC...
We present a new relation between velocity dispersion, surface brightness, and radius (or luminosity...
New surface photometry of all known elliptical galaxies in the Virgo cluster is combined with publis...
This paper reviews surface photometry of bulges and elliptical galaxies. Work prior to 1982 is discu...
Recent results from gravitational lensing are combined with new modeling of the stellar velocity dis...
VizieR online Data Catalogue associated with article published in journal Astronomical Journal (AAS)...
The disks of spiral galaxies are generally elliptical rather than circular. The distribution of elli...
Bright elliptical galaxies have a markedly different distribution of Hubble types than faint ellipti...