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The elliptical galaxy NGC 720: An unequal-mass galaxy merger remnant
- Source :
- Astronomy and Astrophysics; June 2005, Vol. 436 Issue: 1 p57-65, 9p
- Publication Year :
- 2005
-
Abstract
- The stellar population of the central region of the galaxy NGC 720has been investigated through longslit optical spectroscopy. The velocity dispersion and 13 Lick indices were obtained as a function of the radius along the semimajor axis of the galaxy. The Mg2index presents a gradient of ${\rm d\,Mg}_2\,/\,{\rm d\,log}\,r=-0.079$which behaves similarly to the $\ion{Fe}{i}$lines, indicating no enhancement of Mg2in relation to $\ion{Fe}{i}$. The stellar population ages and metallicities were derived by a population synthesis method using available evolutive spectrophotometric models. The synthesis indicates a strong age gradient along the semimajor axis of NGC 720. In the central region a 13 Gyr and solar metallicity stellar population dominates the flux at 5870 Å; the contribution of this component vanishes at a radius of 0.73 kpc, where the total flux is accounted for by a younger, 5 Gyr and solar metallicity stellar population. For distances larger than 1 kpc a 2.5 Gyr component becomes very important. Moreover, NGC 720is probably overabundant in CN in the center with respect to the solar abundance. The estimated total mass ($3.29\times10^{11}~M_\odot$) and the Mg2gradient values suggest that this galaxy might have undergone a merger event. The correspondence between the J-band brightness profile decomposition and the result of the spectral synthesis shows that this galaxy is formed by an old (13–5 Gyr), bulge-like, small-scale and massive spheroid and a younger (5–2.5 Gyr), large-scale disk component. We discuss our results in comparison with available numerical simulations and propose that the merger event must have occurred about 4 Gyr ago.
Details
- Language :
- English
- ISSN :
- 00046361 and 14320746
- Volume :
- 436
- Issue :
- 1
- Database :
- Supplemental Index
- Journal :
- Astronomy and Astrophysics
- Publication Type :
- Periodical
- Accession number :
- ejs53198590
- Full Text :
- https://doi.org/10.1051/0004-6361:20042464