Zobrazeno 1 - 10
of 1 325
pro vyhledávání: '"A. COMERON"'
Autor:
S. Lolli, M. Sicard, F. Amato, A. Comeron, C. Gíl-Diaz, T. C. Landi, C. Munoz-Porcar, D. Oliveira, F. Dios Otin, F. Rocadenbosch, A. Rodriguez-Gomez, A. Alastuey, X. Querol, C. Reche
Publikováno v:
Atmospheric Chemistry and Physics, Vol 23, Pp 12887-12906 (2023)
Aerosols are one of the most important pollutants in the atmosphere and have been monitored for the past few decades by remote sensing and in situ observation platforms to assess the effectiveness of government-managed reduction emission policies and
Externí odkaz:
https://doaj.org/article/4d575dd105b64147b2d473ea76e5072a
Autor:
Murphy, A., Whelan, E. T., Bacciotti, F., Coffey, D., Comerón, F., Eislöffel, J., Nisini, B., Antoniucci, S., Alcalá, J. M., Ray, T. P.
Publikováno v:
Astronomy and Astrophysics 691 (2024) A48
Characterising stellar jet asymmetries is key to setting robust constraints on jet launching models and improving our understanding of the underlying mechanisms behind jet launching. We aim to characterise the asymmetric properties of the bipolar jet
Externí odkaz:
http://arxiv.org/abs/2411.12269
Autor:
Sattler, Natascha, Pinna, Francesca, Comerón, Sebastien, Martig, Marie, Falcón-Barroso, Jesus, Martín-Navarro, Ignacio, Neumayer, Nadine
We aim to trace the evolution of eight edge-on star-forming disc galaxies through the analysis of stellar population properties of their thin and thick discs. These galaxies have relatively low stellar masses (4 $\times$ 10$^9$ to 6 $\times$ 10$^{10}
Externí odkaz:
http://arxiv.org/abs/2410.05761
Autor:
Mulumba, Dorcus, Knapen, Johan, Comeron, Sebastien, Almeida, Cristina Ramos, Obonyo, Willice, Santaella, Pereira, Baki, Paul
Understanding how gas flows into galactic centres, fuels the AGN, and is in turn expelled back through feedback processes is of great importance to appreciate the role AGN play in the growth and evolution of galaxies. We use the MUSE-AO optical spect
Externí odkaz:
http://arxiv.org/abs/2410.03110
The ionization of diffuse gas located far above the energetic midplane OB stars poses a challenge to the commonly accepted notion that radiation from OB stars is the primary ionization source for gas in galaxies. We investigated the sources of ionizi
Externí odkaz:
http://arxiv.org/abs/2409.16062
Highly inclined (edge-on) disk galaxies offer the unique perspective to constrain their intrinsic flattening, $c/a$, where $c$ and $a$ are respectively the vertical and long radial axes of the disk measured at suitable stellar densities. The ratio $c
Externí odkaz:
http://arxiv.org/abs/2409.06768
Autor:
Amiri, Amirnezam, Knapen, Johan H., Comerón, Sébastien, Marconi, Alessandro, Lehmer, Bret. D.
Publikováno v:
A&A 689, A193 (2024)
Metallicity measurements in galaxies can give valuable clues about galaxy evolution. One of the mechanisms postulated for metallicity redistribution in galaxies is gas flows induced by AGN, but the details of this process remain elusive. We report th
Externí odkaz:
http://arxiv.org/abs/2407.12158
Publikováno v:
Open Journal of Astrophysics, Vol. 7, 2024
We investigate the star formation occurring in the Planck Galactic cold clump PGCC 120.69+2.66. Near-infrared JHKs images and K-band spectroscopy obtained with NOTCam at the Nordic Optical Telescope complemented with archive data are used to study th
Externí odkaz:
http://arxiv.org/abs/2405.15469
Autor:
Dib, Sami, Zhou, Jian Wen, Comerón, Sébastien, Garduño, Luis E., Kravtsov, Valery V., Clark, Paul C., Li, Guang-Xing, Lara-López, Maritza A., Liu, Tie, Shadmehri, Mohsen, Doughty, James R.
Star formation estimates based on the counting of YSOs is commonly applied to nearby star-forming regions in the Galaxy. With this method, the SFRs are measured using the counts of YSOs in a particular protostellar Class, a typical protostellar mass,
Externí odkaz:
http://arxiv.org/abs/2405.00095
Autor:
Schneider, N., Ossenkopf-Okada, V., Keilmann, E., Roellig, M., Kabanovic, S., Bonne, L., Csengeri, T., Klein, B., Simon, R., Comeron, F.
High-latitude intermediate-velocity clouds (IVCs) are part of the Milky Way's HI halo and originate from either a galactic fountain process or extragalactic gas infall. They are partly molecular and can most of the time be identified in CO. Some of t
Externí odkaz:
http://arxiv.org/abs/2404.15739