Results 21 to 30 of about 314 (90)
Structural and dynamical modeling of WINGS clusters [PDF]
Astronomy & Astrophysics, 2019 The orbital shapes of galaxies of different classes are a probe of their formation and evolution. The Bayesian MAMPOSSt mass-orbit modeling algorithm is used to jointly fit the distribution of elliptical, spiral-irregular, and lenticular galaxies in projected phase space, on three pseudo-clusters (built by stacking the clusters after re-normalizing ...
G. A. Mamon +5 more
openaire +6 more sources
The Dynamical Distinction between Elliptical and Lenticular Galaxies in Distant Clusters: Further Evidence for the Recent Origin of S0 Galaxies [PDF]
The Astrophysical Journal, 2007 We examine resolved spectroscopic data obtained with the Keck II telescope for 44 spheroidal galaxies in the fields of two rich clusters, Cl0024+16 (z=0.40) and MS0451-03 (z=0.54), and contrast this with similar data for 23 galaxies within the redshift interval 0 ...
Moran, Sean M. +5 more
openaire +5 more sources
Multicolor surface photometry of lenticular galaxies. I. The data [PDF]
, 2005 We present multicolor surface and aperture photometry in the B, V, R, and K' bands for a sample of 34 lenticular galaxies from the Uppsala General Catalogue.
Pandey, S. K. +3 more
core +1 more source
The Cool ISM in Elliptical Galaxies. II. Gas Content in the Volume - Limited Sample and Results from the Combined Elliptical and Lenticular Surveys [PDF]
The Astrophysical Journal, 2010 37 pages, including 4 tables and 12 figures.
Welch, Gary A. +2 more
openaire +3 more sources
Properties of the Photometric Components of Lenticular Galaxies
Advances in Astronomy, Volume 2012, Issue 1, 2012., 2012 After almost one century since their definition, the origin of lenticular galaxies is still a matter of debate. Several formation processes have been proposed in order to explain the wide variety of their observational properties. These properties could indicate that the class of lenticulars is a family formed by galaxies with different formations and ...
J. Alfonso L. Aguerri, Elias Brinks
wiley +1 more source
Implications and Applications of Kinematic Galaxy Scaling Relations
International Scholarly Research Notices, Volume 2012, Issue 1, 2012., 2012 Galaxy scaling relations, which describe a connection between ostensibly unrelated physical characteristics, testify to an underlying order in galaxy formation that requires understanding. I review the development of a scaling relation that (1) unites the well‐known fundamental plane (FP) relation of giant elliptical galaxies and Tully‐Fisher (TF ...
Dennis Zaritsky +2 more
wiley +1 more source
The present-day galaxy population in spiral galaxies [PDF]
, 2009 Although there are many more stellar population studies of elliptical and lenticular galaxies, studies of spiral galaxies are catching up, due to higher signal to noise data on one hand, and better analysis methods on the other.
Enzo Brocato +9 more
core +2 more sources
The Astrophysical Journal, 1982 The Faber-Jackson relation between absolute magnitude M/sub T//sup 0/ and central velocity dispersion sigma/sub upsilon/ is reexamined for a sample of 157 normal, noninteracting galaxies, 82 ellipticals (T = -5, -4), and 75 lenticulars (T = -3, -2, -1). The values of sigma/sub upsilon/ are weighted means from various sources reduced to a uniform system
G. de Vaucouleurs, D. W. Olson
openaire +1 more source
Chromodynamical analysis of lenticular galaxies using globular clusters and planetary nebulae [PDF]
, 2018 Recovering the origins of lenticular galaxies can shed light on the understanding of galaxy formation and evolution, since they present properties that can be found in both elliptical and spiral galaxies.
Coccato, Lodovico +20 more
core +1 more source
Extended stellar kinematics of elliptical galaxies in the Fornax cluster?;?? [PDF]
, 1998 . We present extended stellar kinematics for a sample of elliptical galaxies in the Fornax cluster. Out of the 13 galaxies presented here, ve (FCC 119, FCC 136, NGC 1373, NGC 1428, FCC 335) have no pre-viously published kinematical data.
Longo, G +9 more
core +1 more source