Zobrazeno 1 - 10
of 639
pro vyhledávání: '"Sarzi M"'
Autor:
Castelli, A. V. Smith, Cortesi, A., Haack, R. F., Lopes, A. R., Thainá-Batista, J., Fernandes, R. Cid, Lomelí-Núñez, L., Ribeiro, U., de Bom, C. R., Cernic, V., Sodré Jr, L., Zenocratti, L., De Rossi, M. E., Calderón, J. P., Herpich, F., Telles, E., Saha, K., Lopes, P. A. A., Lopes-Silva, V. H., Gonçalves, T. S., Bambrila, D., Cardoso, N. M., Buzzo, M. L., Sotomayor, P. Astudillo, Demarco, R., Leigh, N., Sarzi, M., Menéndez-Delmestre, K., Faifer, F. R., Jiménez-Teja, Y., Grossi, M., Hernández-Jiménez, J. A., Krabbe, A. C., Soto, L. A. Gutiérrez, Brandão, D., Espinosa, L., Olave-Rojas, D. E., Schwarz, G. B. Oliveira, Almeida-Fernandes, F., Schoenell, W., Ribeiro, T., Kanaan, A., de Oliveira, C. Mendes
The Fornax galaxy cluster is the richest nearby (D ~ 20 Mpc) galaxy association in the southern sky. As such, it provides a wealth of oportunities to elucidate on the processes where environment holds a key role in transforming galaxies. Although it
Externí odkaz:
http://arxiv.org/abs/2403.10697
Autor:
Hagedorn, B., Cicone, C., Sarzi, M., Saintonge, A., Severgnini, P., Vignali, C., Shen, S., Rubinur, K., Schimek, A., Lasrado, A.
Publikováno v:
A&A 687, A244 (2024)
We derived molecular gas fractions ($f_\mathrm{mol}=M_\mathrm{mol}/M_*$) and depletion times ($\tau_\mathrm{mol}= M_\mathrm{mol}/\mathrm{SFR} $) for 353 galaxies representative of the local star-forming population with $10^{8.5}\,M_\odot < M_* < 10^{
Externí odkaz:
http://arxiv.org/abs/2402.18291
Autor:
Ding, Y., Zhu, L., van de Ven, G., Coccato, L., Corsini, E. M., Costantin, L., Fahrion, K., Falcón-Barroso, J., Gadotti, D. A., Iodice, E., Lyubenova, M., Martín-Navarro, I., McDermid, R. M., Pinna, F., Sarzi, M.
Publikováno v:
A&A 672, A84 (2023)
We apply a population-orbit superposition method to 16 galaxies in the Fornax cluster observed with MUSE/VLT in the context of the Fornax3D project. By fitting the luminosity distribution, stellar kinematics, and age and metallicity maps simultaneous
Externí odkaz:
http://arxiv.org/abs/2301.05532
Autor:
Anta, Pablo M. Galán-de, Sarzi, M., Pillepich, A., Ding, Y., Zhu, L., Coccato, L., Corsini, E. M., Fahrion, K., Falcón-Barroso, J., Gadotti, D. A., Iodice, E., Lyubenova, M., Martín-Navarro, I., McDermid, R. M., Pinna, F., van de Ven, G., de Zeeuw, P. T.
We study the evolution of kinematically-defined stellar discs in 10 Fornax-like clusters identified in the TNG50 run from the IllustrisTNG suite of cosmological simulations. We considered disc galaxies with present-day stellar mass $M_{\star}\geq 3 \
Externí odkaz:
http://arxiv.org/abs/2211.00429
Autor:
Spavone, M., Iodice, E., D'Ago, G., van de Ven, G., Morelli, L., Corsini, E. M., Sarzi, M., Coccato, L., Fahrion, K., Falcón-Barroso, J., Gadotti, D. A., Lyubenova, M., Martín-Navarro, I., McDermid, R. M., Pinna, F., Pizzella, A., Poci, A., de Zeeuw, P. T., Zhu, L.
Publikováno v:
A&A 663, A135 (2022)
This work is based on high quality integral-field spectroscopic data obtained with the Multi Unit Spectroscopic Explorer (MUSE) on the Very Large Telescope (VLT). The 21 brightest ($m_B\leq 15$ mag) early-type galaxies (ETGs) inside the virial radius
Externí odkaz:
http://arxiv.org/abs/2205.15331
Autor:
Poci, A., McDermid, R. M., Lyubenova, M., Martin-Navarro, I., van de Ven, G., Coccato, L., Corsini, E. M., Fahrion, K., Falcon-Barroso, J., Gadotti, D. A., Iodice, E., Pinna, F., Sarzi, M., de Zeeuw, P. T., Zhu, L.
[arXiv Abridged] In this work, we explore new spatially-resolved measurements of the IMF for three edge-on lenticular galaxies in the Fornax cluster. Specifically, we utilise existing orbit-based dynamical models, which re-produce the measured stella
Externí odkaz:
http://arxiv.org/abs/2205.13082
Autor:
Lara-Lopez, M. A., Anta, P. M. Galan-de, Sarzi, M., Iodice, E., Davis, T. A., Zabel, N., Corsini, E. M., de Zeeuw, P. T., Fahrion, K., Falcon-Barroso, J., Gadotti, D. A., McDermid, R. M., Pinna, F., Rodriguez-Gomez, V., van de Ven, G., Zhu, L., Coccato, L., Lyubenova, M., Martin-Navarro, I.
Publikováno v:
A&A 660, A105 (2022)
The role played by environment in galaxy evolution is a current debate in astronomy. The degree to which environment can alter, re-shape, or drive galaxy evolution is a topic of discussion in both fronts, observations and simulations. This paper anal
Externí odkaz:
http://arxiv.org/abs/2202.04128
Autor:
Mernier, F., Werner, N., Su, Y., Pinto, C., Grossová, R., Simionescu, A., Iodice, E., Sarzi, M., Görgei, A.
Hot atmospheres pervading galaxy clusters, groups, and early-type galaxies are rich in metals, produced during epochs and diffused via processes that are still to be determined. While this enrichment has been routinely investigated in clusters, metal
Externí odkaz:
http://arxiv.org/abs/2201.05161
Autor:
Martín-Navarro, I., Pinna, F., Coccato, L., Falcón-Barroso, J., van de Ven, G., Lyubenova, M., Corsini, E. M., Fahrion, K., Gadotti, D. A., Iodice, E., McDermid, R. M., Poci, A., Sarzi, M., Spriggs, T. W., Viaene, S., de Zeeuw, P. T., Zhu, L.
Publikováno v:
A&A 654, A59 (2021)
The stellar initial mass function (IMF) is central to our interpretation of astronomical observables and to our understanding of most baryonic processes within galaxies. The universality of the IMF, suggested by observations in our own Milky Way, has
Externí odkaz:
http://arxiv.org/abs/2107.14243
Autor:
Anta, P. M. Galán-de, Sarzi, M., Spriggs, T. W., Nedelchev, B., Pinna, F., Martín-Navarro, I., Coccato, L., Corsini, E. M., de Zeeuw, P. T., Falcón-Barroso, J., Gadotti, D. A., Iodice, E., Grand, R. J. J., Fahrion, K., Lyubenova, M., McDermid, R. M., Morelli, L., van de Ven, G., Viaene, S., Zhu, L.
Publikováno v:
A&A 652, A109 (2021)
Context. Extragalactic Planetary Nebulae (PNe) are useful distance indicators and are often used to trace the dark-matter content in external galaxies. At the same time, PNe can also be used as probes of their host galaxy stellar populations and to h
Externí odkaz:
http://arxiv.org/abs/2106.11657