Results 11 to 20 of about 242,935 (158)

NGC 1436: the making of a lenticular galaxy in the Fornax cluster [PDF]

open access: greenMonthly notices of the Royal Astronomical Society, 2023
We study the evolutionary path of the Fornax cluster galaxy NGC 1436, which is known to be currently transitioning from a spiral into a lenticular morphology. This galaxy hosts an inner star-forming disc and an outer quiescent disc, and we analyse data
A. Loni   +28 more
semanticscholar   +2 more sources

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

open access: diamondAstronomy & Astrophysics, 2022
Aims. We characterised the properties of the bar hosted in lenticular galaxy NGC4277, 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 ...
C. Buttitta   +11 more
semanticscholar   +2 more sources

The present-day globular cluster kinematics of lenticular galaxies from the E-MOSAICS simulations and their relation to the galaxy assembly histories [PDF]

open access: bronzeMonthly notices of the Royal Astronomical Society, 2022
We study the present-day rotational velocity (Vrot) and velocity dispersion (σ) profiles of the globular cluster (GC) systems in a sample of 50 lenticular (S0) galaxies from the E-MOSAICS galaxy formation simulations.
A. Dolfi   +7 more
semanticscholar   +3 more sources

WISDOM Project – IX. Giant molecular clouds in the lenticular galaxy NGC 4429: effects of shear and tidal forces on clouds [PDF]

open access: hybridMonthly notices of the Royal Astronomical Society, 2021
We present high spatial resolution (≈12 pc) Atacama Large Millimeter/submillimeter Array 12CO(J = 3–2) observations of the nearby lenticular galaxy NGC 4429. We identify 217 giant molecular clouds within the 450 pc radius molecular gas disc. The clouds
Lijie Liu   +7 more
semanticscholar   +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.
N. Boardman   +10 more
semanticscholar   +3 more sources

The MBHBM$^{\star}$ Project -- II. Molecular Gas Kinematics in the Lenticular Galaxy NGC 3593 Reveal a Supermassive Black Hole [PDF]

open access: green, 2021
As part of the Measuring Black Holes in BelowMilkyWay-mass (M) galaxies (MBHBM) Project, we present a dynamical measurement of the supermassive black hole (SMBH) mass in the nearby lenticular galaxy NGC 3593, using cold molecular gas 12CO(2-1) emission ...
Dieu D. Nguyen   +17 more
semanticscholar   +3 more sources

The SLUGGS survey: chromodynamical modelling of the lenticular galaxy NGC 1023 [PDF]

open access: bronze, 2015
Globular clusters (GCs) can be considered discrete, long-lived, dynamical tracers that retain crucial information about the assembly history of their parent galaxy. In this paper, we present a new catalogue of GC velocities and colours for the lenticular
A. Cortesi   +14 more
semanticscholar   +3 more sources

S-PLUS: LEnticular Galaxies in Stripe 82 (LEGS82) [PDF]

open access: diamondAnais da Academia Brasileira de Ciências, 2021
This work is a Brazilian-Indian collaboration. It aims at investigating the structural properties of Lenticular galaxies in the Stripe 82 using a combination of S-PLUS (Southern Photometric Local Universe Survey) and SDSS data.
ARIANNA CORTESI   +7 more
doaj   +4 more sources

Fornax 3D project: a two-dimensional view of the stellar initial mass function in the massive lenticular galaxy FCC 167 [PDF]

open access: bronzeAstronomy & Astrophysics, 2019
The stellar initial mass function (IMF) regulates the baryonic cycle within galaxies, and is a key ingredient for translating observations into physical quantities.
I. Martín-Navarro   +14 more
semanticscholar   +3 more sources

A Chandra Observation of the Nearby Lenticular Galaxy NGC 5102: Where Are the X-Ray Binaries? [PDF]

open access: bronze, 2005
We present results from a 34 ks Chandra ACIS-S observation of the low-mass X-ray binary (LMXB) population and the hot interstellar medium (ISM) in the nearby (d = 3.1 Mpc) lenticular galaxy NGC 5102, previously shown to have an unusually low X-ray ...
R. Kraft   +4 more
semanticscholar   +3 more sources

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