Results 81 to 90 of about 6,480 (173)
Photometric scaling relations of lenticular and spiral galaxies [PDF]
Accepted to MNRAS, includes a big figure in electronic form, not included ...
Laurikainen, E. +4 more
openaire +2 more sources
PGC 44685: A Dwarf Star-forming Lenticular Galaxy with a Wolf–Rayet Population
Lenticular galaxies (S0s) are formed mainly from the gas stripping of spirals in the cluster. But how S0s form and evolve in the field is still in need of being resolved.
Shiying Lu +10 more
doaj +1 more source
Structure of the Galaxies in the NGC 80 Group [PDF]
BV-bands photometric data obtained at the 6-m telescope of the Special Astrophysical Observatory are used to analyze the structure of 13 large disk galaxies in the NGC 80 group.
A. Dressler +43 more
core +1 more source
Faint Fuzzies and the Formation of Lenticular Galaxies [PDF]
11 pages, 4 figures, ApJ, in ...
Burkert, A., Brodie, J., Larsen, S.
openaire +3 more sources
A gaseous counterrotating galaxy is a galaxy containing a gas component with opposite angular momentum to the main stellar disk. The counterrotating gas provides direct evidence for the accretion of external material, a key aspect in hierarchical galaxy ...
Minje Beom +2 more
doaj +1 more source
Radio Jet Feedback on the Inner Disk of Virgo Spiral Galaxy Messier 58
Spitzer spectral maps reveal a disk of highly luminous, warm (>150 K) H _2 in the center of the massive spiral galaxy Messier 58, which hosts a radio-loud active galactic nucleus (AGN). The inner 2.6 kpc of the galaxy appears to be overrun by shocks from
Patrick M. Ogle +11 more
doaj +1 more source
Combining Chandra, Atacama Large Millimeter/submillimeter Array, EVLA, and Hubble Space Telescope archival data and newly acquired data from the Apache Point Observatory/Dual Imaging Spectrograph, we detect a double-lobed 17 kpc X-ray emission with ...
Alejandro S. Borlaff +13 more
doaj +1 more source
The Cool ISM in S0 Galaxies. I. A Survey of Molecular Gas
Lenticular galaxies remain remarkably mysterious as a class. Observations to date have not led to any broad consensus about their origins, properties and evolution, though they are often thought to have formed in one big burst of star formation early in ...
Appleton P. N. +37 more
core +2 more sources
Minor-merger-induced Star Formation Rejuvenation in an Elliptical Radio-loud Quasar Host, 3C 59
We report a rare case where an elliptical radio-loud quasar host, 3C 59, rejuvenates star formation activity through minor mergers with its nearby satellite galaxies.
Yijun Wang +5 more
doaj +1 more source
Modelling the photometric and morphological evolution of disc galaxies in the cluster environment
Compelling observational evidence indicates that the disc population in galaxy clusters has undergone rapid evolution, transitioning from a dominance of blue spirals to red lenticular galaxies (S0s) over the past ∼7 Gyr.
Marasco A. +5 more
doaj +1 more source

