Clues to the Formation of Lenticular Galaxies Using Spectroscopic Bulge-Disk Decomposition [PDF]
arXiv, 2013 Lenticular galaxies have long been thought of as evolved spirals, but the processes involved to quench the star formation are still unclear. By studying the individual star formation histories of the bulges and disks of lenticulars, it is possible to look for clues to the processes that triggered their transformation from spirals.
arxiv
The SAURON project – VIII. OASIS/CFHT integral-field spectroscopy of elliptical and lenticular galaxy centres* [PDF]
, 2006 Richard M. McDermid +12 more
openalex +1 more source
The H I content of elliptical and lenticular galaxies withrecent star formation [PDF]
, 2007 J. F. Helmboldt
openalex +1 more source
Repainting the colour-mass diagrams by unearthing the green mountain: dust-rich S0 galaxies in the colour-(galaxy stellar mass) diagram, and the colour-(black hole mass) relations for dust-poor versus dust-rich galaxies [PDF]
arXivLenticular galaxies are notoriously misclassified as elliptical galaxies and, as such, a (disc inclination)-dependent correction for dust is often not applied to the magnitudes of dusty lenticular galaxies. This results in overly red galaxy colours, impacting their distribution in the colour-magnitude diagram.
arxiv
The lenticular galaxy NGC 3607: stellar population, metallicity, and ionised gas [PDF]
, 2009 M. G. Rickes +2 more
openalex +1 more source
The Astronomical JournalA 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
A common colour-magnitude relation from giant elliptical galaxies to globular clusters? [PDF]
arXiv, 2009 We discuss the existence of a common colour-magnitude relation (CMR) of metal-poor globular clusters and early-type galaxies, i.e. giant ellipticals, normal ellipticals and lenticulars, dwarf ellipticals and lenticulars, and dwarf spheroidals. Such CMR would cover a range of ~ 14 mag, extending from the brightest galaxies, down to the globular clusters
arxiv
Biomimetic Nanomembranes: An Overview. [PDF]
Biomimetics (Basel), 2020 Jakšić Z, Jakšić O.
europepmc +1 more source
Evidence for Mass-dependent Evolution of Transitional Dwarf Galaxies in the Virgo Cluster
The Astrophysical JournalThe presence of transitional dwarf galaxies in cluster environments supports the hypothesis that infalling star-forming galaxies are transformed into quiescent early-type dwarf galaxies (ETdGs) through environmental effects.
Suk Kim, Soo-Chang Rey, Youngdae Lee
doaj +1 more source
Asymmetric Star Formation Triggered by Gas Inflow in a Barred Lenticular Galaxy PGC 34107
, 2022 Shiying Lu +10 more
openalex +1 more source