Zobrazeno 1 - 10
of 993
pro vyhledávání: '"Contini M."'
We study the ionised and highly ionised gas phases in the Seyfert~2 galaxy IC~5063 by means of VLT/MUSE integral field spectroscopy. Our analysis allowed us to detect a high-ionisation gas outflow traced by the coronal lines [\ion{Fe}{vii}]~$\lambda$
Externí odkaz:
http://arxiv.org/abs/2306.09570
Publikováno v:
In Tissue and Cell June 2024 88
We employ MUSE/VLT data to study the ionised and highly ionised gas phases of the feedback in Circinus, the closest Seyfert 2 galaxy to us. The analysis of the nebular emission allowed us to detect a remarkable high-ionisation gas outflow beyond the
Externí odkaz:
http://arxiv.org/abs/2106.13324
Publikováno v:
In General and Comparative Endocrinology 1 March 2024 348
Autor:
Dors, O. L., Contini, M., Riffel, R. A., Perez-Montero, E., Krabbe, A. C., Cardaci, M. V., Hagele, G. F.
We build detailed composite models of photoionization and shock ionization based on the SUMA code to reproduce emission lines emitted from the Narrow Line Regions (NLR) of Seyfert 2 nuclei. The aim of this work is to investigate diagram AGN positions
Externí odkaz:
http://arxiv.org/abs/2011.12103
Autor:
Contini, M.
We have modelled the line ratios and the continuum spectral energy distribution (SED) of the short gamma-ray burst GRB100628A host galaxy complex. The results suggest that an active galactic nucleus (AGN) and a star-burst (SB) coexist in Nicuesa Guel
Externí odkaz:
http://arxiv.org/abs/1908.05157
Autor:
Congiu, E., Contini, M., Ciroi, S., Cracco, V., Berton, M., Di Mille, F., Frezzato, M., La Mura, G., Rafanelli, P.
We studied the properties of the gas of the extended narrow line region (ENLR) of two Seyfert 2 galaxies: IC 5063 and NGC 7212. We analysed high resolution spectra to investigate how the main properties of this region depend on the gas velocity. We d
Externí odkaz:
http://arxiv.org/abs/1706.08970
Autor:
Contini, M.
The distribution of N/O abundance ratios calculated by the detailed modelling of different galaxy spectra at z<4 is investigated. Supernova (SN) and long gamma-ray-burst (LGRB) host galaxies cover different redshift domains. N/O in SN hosts increases
Externí odkaz:
http://arxiv.org/abs/1704.07604
Autor:
Contini, M.
We revisited the line spectra emitted from long GRB (LGRB) host galaxies at z<0.5 in order to calculate by the detailed modelling of the line ratios the physical conditions and relative abundances in LGRB hosts in this redshift range. We have found l
Externí odkaz:
http://arxiv.org/abs/1612.03387
Autor:
Contini, M.
We analyze by detailed modelling the spectra observed from the sample galaxies at z$\sim$0.8 presented by Ly et al (2015), constraining the models by the [OIII]5007+4959/[OIII]4363 line ratios. Composite models accounting for shock and photoionizatio
Externí odkaz:
http://arxiv.org/abs/1606.04667