We present new central stellar velocity dispersion measurements for 428 galaxies in the Palomar spectroscopic survey of bright, northern galaxies. Of these, 142 have no previously published measurements, most being rela-tively late-type systems with low velocity dispersions (∼<100 km s−1). We provide updates to a number of literature dispersions with large uncertainties. Our measurements are based on a direct pixel-fitting technique that can ac-commodate composite stellar populations by calculating an optimal linear combination of input stellar templates. The original Palomar survey data were taken under conditions that are not ideally suited for deriving stellar veloc-ity dispersions for galaxies with a wide range of Hubble types. We de...
We present central velocity dispersions and Mg2 line indices for an all-sky sample of ~1178 elliptic...
The distribution of early-type galaxy velocity dispersions, phgr(σ), is measured using a sample draw...
We have carried out a systematic, homogeneous comparison of optical and near-infrared dis-persions. ...
We present new central stellar velocity dispersion measurements for 428 galaxies in the Palomar spec...
SUMMARY: We present the central velocity dispersion measurements of the nearby galaxies from the Slo...
We present the central velocity dispersion measurements of the nearby galaxies from the Sloan Digita...
We define a large sample of galaxies for use in a study of the fundamental plane in the intermediate...
We analyze the kinematics of the central regions of five isolated Seyfert spiral galaxies from the D...
The velocity distribution of galaxies in clusters is not universal; rather, galaxies are segregated ...
Context. Current spectroscopic and photometric surveys are providing a comprehensive view of the Mil...
We present the study of a large sample of early-type dwarf galaxies in the Coma cluster observed wit...
We analyze the kinematics of the central regions of five isolated Seyfert spiral galaxies from the D...
An analysis of large-area CO J = 3-2 maps from the James Clerk Maxwell Telescope for 12 nearby spira...
We examine the stellar velocity dispersions (sigma) of a sample of 48 galaxies, 35 of which are spir...
Long slit absorption line spectroscopy has been obtained of the close to face-on Sc galaxy NGC 1566 ...
We present central velocity dispersions and Mg2 line indices for an all-sky sample of ~1178 elliptic...
The distribution of early-type galaxy velocity dispersions, phgr(σ), is measured using a sample draw...
We have carried out a systematic, homogeneous comparison of optical and near-infrared dis-persions. ...
We present new central stellar velocity dispersion measurements for 428 galaxies in the Palomar spec...
SUMMARY: We present the central velocity dispersion measurements of the nearby galaxies from the Slo...
We present the central velocity dispersion measurements of the nearby galaxies from the Sloan Digita...
We define a large sample of galaxies for use in a study of the fundamental plane in the intermediate...
We analyze the kinematics of the central regions of five isolated Seyfert spiral galaxies from the D...
The velocity distribution of galaxies in clusters is not universal; rather, galaxies are segregated ...
Context. Current spectroscopic and photometric surveys are providing a comprehensive view of the Mil...
We present the study of a large sample of early-type dwarf galaxies in the Coma cluster observed wit...
We analyze the kinematics of the central regions of five isolated Seyfert spiral galaxies from the D...
An analysis of large-area CO J = 3-2 maps from the James Clerk Maxwell Telescope for 12 nearby spira...
We examine the stellar velocity dispersions (sigma) of a sample of 48 galaxies, 35 of which are spir...
Long slit absorption line spectroscopy has been obtained of the close to face-on Sc galaxy NGC 1566 ...
We present central velocity dispersions and Mg2 line indices for an all-sky sample of ~1178 elliptic...
The distribution of early-type galaxy velocity dispersions, phgr(σ), is measured using a sample draw...
We have carried out a systematic, homogeneous comparison of optical and near-infrared dis-persions. ...