Results 21 to 30 of about 372,374 (202)

Abundant Molecular Gas in the Central Region of Lenticular Galaxy PGC 39535 [PDF]

open access: yesThe Astrophysical Journal
Lenticular galaxies (S0s) in the local Universe are generally absent of recent star formation and lack molecular gas. In this paper, we investigate one massive ( M _* ∼ 5 × 10 ^10 M _⊙ ) star-forming S0, PGC 39535, with the Northern Extended Millimeter ...
Jiantong Cui   +5 more
doaj   +2 more sources

Luminosities of Barred and Unbarred S0 Galaxies [PDF]

open access: yes, 2012
Lenticular galaxies with M_B < -21.5 are almost exclusively unbarred, whereas both barred and unbarred objects occur at fainter luminosity levels. This effect is observed both for objects classified in blue light, and for those that were classified in ...
Buta   +9 more
core   +2 more sources

Elliptical (E) and ellicular (ES) galaxies in the M_bh-M_*,sph diagram, and a merger-driven explanation for the origin of ES galaxies, anti-truncated stellar discs in lenticular galaxies, and the Sersicification of E galaxy light profiles [PDF]

open access: yesMNRAS (2024) v.535, p.299
In a recent series of papers, supermassive black holes were used to discern pathways in galaxy evolution. By considering the black holes' coupling with their host galaxy's bulge/spheroid, the progression of mass within each component has shed light on the chronological sequence of galaxy speciation.
A. Graham
arxiv   +3 more sources

A slow bar in the lenticular barred galaxy NGC 4277 [PDF]

open access: yesAstronomy & Astrophysics, 2022
Aims.We characterised the properties of the bar hosted in lenticular galaxy NGC 4277, which is located behind the Virgo cluster.Methods.We measured the bar length and strength from the surface photometry obtained from the broad-band imaging of the Sloan Digital Sky Survey and we derived the bar pattern speed from the stellar kinematics obtained from ...
Buttitta, C.   +11 more
openaire   +4 more sources

Faint Fuzzies and the Formation of Lenticular Galaxies [PDF]

open access: bronzeThe Astrophysical Journal, 2005
11 pages, 4 figures, ApJ, in ...
Andreas Burkert   +2 more
openalex   +7 more sources

Photometric scaling relations of lenticular and spiral galaxies [PDF]

open access: hybridMonthly Notices of the Royal Astronomical Society, 2010
Accepted to MNRAS, includes a big figure in electronic form, not included ...
E. Laurikainen   +4 more
openalex   +6 more sources

Inner structure of the lenticular galaxy NGC 3384 [PDF]

open access: bronzeMonthly Notices of the Royal Astronomical Society, 1984
La region interne de la galaxie lenticulaire NGC 3384 presente une structure complexe. La haute resolution (FWHM≃0,7 arc sec) obtenue pour cette etude photometrique permet de montrer que la faible structure allongee croisant le bulbe perpendiculairement a l'axe principal de la galaxie n'est probablement pas une barre, mais un petit anneau polaire de ...
E. Davoust   +3 more
openalex   +3 more sources

The low dark matter content of the lenticular galaxy NGC 3998 [PDF]

open access: bronze, 2016
We observed the lenticular galaxy NGC 3998 with the Mitchell Integral-Field Spectrograph and extracted line-of-sight velocity distributions out to 3 half-light radii.
Nicholas Fraser Boardman   +10 more
openalex   +3 more sources

Inner Polar Rings in Regular Lenticular Galaxies [PDF]

open access: bronzeThe Astronomical Journal, 2004
We have investigated a sample of S0 galaxies, mostly with circumnuclear dust lanes orthogonal to their major axes, chosen from Hubble Space Telescope Wide Field Planetary Camera 2 images. Two-dimensional spectroscopy undertaken with the Multipupil Fiber Spectrograph of the 6 m telescope of the Special Astrophysical Observatory of the Russian Academy of
О. К. Сильченко   +1 more
openalex   +3 more sources

Exponential bulges and antitruncated disks in lenticular galaxies [PDF]

open access: yesProceedings of the International Astronomical Union, 2008
The presence of exponential bulges and anti-truncated disks has been noticed in many lenticular galaxies. In fact, it could be expected because the very formation of S0 galaxies includes various processes of secular evolution. We discuss how to distinguish between a pseudobulge and an anti-truncated disk, and also what particular mechanisms may be ...
arxiv   +5 more sources

Home - About - Disclaimer - Privacy