2017A&A...600A..76M


Query : 2017A&A...600A..76M

2017A&A...600A..76M - Astronomy and Astrophysics, volume 600A, 76-76 (2017/4-1)

Kinematic and stellar population properties of the counter-rotating components in the S0 galaxy NGC 1366.

MORELLI L., PIZZELLA A., COCCATO L., CORSINI E.M., DALLA BONTA E., BUSON L.M., IVANOV V.D., PAGOTTO I., POMPEI E. and ROCCO M.

Abstract (from CDS):

Context. Many disk galaxies host two extended stellar components that rotate in opposite directions. The analysis of the stellar populations of the counter-rotating components provides constraints on the environmental and internal processes that drive their formation.
Aims. The S0 NGC 1366 in the Fornax cluster is known to host a stellar component that is kinematically decoupled from the main body of the galaxy. Here we successfully separated the two counter-rotating stellar components to independently measure the kinematics and properties of their stellar populations.
Methods. We performed a spectroscopic decomposition of the spectrum obtained along the galaxy major axis and separated the relative contribution of the two counter-rotating stellar components and of the ionized-gas component. We measured the line-strength indices of the two counter-rotating stellar components and modeled each of them with single stellar population models that account for the α/Fe overabundance.
Results. We found that the counter-rotating stellar component is younger, has nearly the same metallicity, and is less α/Fe enhanced than the corotating component. Unlike most of the counter-rotating galaxies, the ionized gas detected in NGC 1366 is neither associated with the counter-rotating stellar component nor with the main galaxy body. On the contrary, it has a disordered distribution and a disturbed kinematics with multiple velocity components observed along the minor axis of the galaxy.
Conclusions. The different properties of the counter-rotating stellar components and the kinematic peculiarities of the ionized gas suggest that NGC 1366 is at an intermediate stage of the acquisition process, building the counter-rotating components with some gas clouds still falling onto the galaxy.

Abstract Copyright: © ESO, 2017

Journal keyword(s): galaxies: abundances - galaxies: kinematics and dynamics - galaxies: formation - galaxies: stellar content - galaxies: individual: 1366 - galaxies: individual: 1366

Simbad objects: 4

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Number of rows : 4
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024
#notes
1 NGC 1366 Sy2 03 33 53.6940996096 -31 11 38.966332632   12.94   11.49   ~ 92 0
2 ACO S 373 ClG 03 38 29.4 -35 27 08           ~ 1794 0
3 NGC 4138 Sy2 12 09 29.8011417048 +43 41 06.864140004 12.46 12.29 11.32 10.82   ~ 402 1
4 NGC 4550 GiP 12 35 30.5913588048 +12 13 14.921166792 12.97 12.56 11.68     ~ 532 1

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2023.11.28-11:32:41

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