Ultraviolet/Optical Emission of the Ionized Gas in AGN: Diagnostics of the Ionizing Source and Gas Properties

Autor: Anna Feltre, Stephane Charlot, Marco Mignoli, Angela Bongiorno, Francesco Calura, Jacopo Chevallard, Emma Curtis-Lake, Roberto Gilli, Adele Plat

Publikováno v: Frontiers in Astronomy and Space Sciences, Vol 4 (2017)

Spectroscopic studies of active galactic nuclei (AGN) are powerful means of probing the physical properties of the ionized gas within them. In particular, near future observational facilities, such as the James Webb Space Telescope (JWST), will allow

Externí odkaz: https://doaj.org/article/8b95604e87dd46a89ab43a02d9f63515

The resolved scaling relations in DustPedia: Zooming in on the local Universe

Autor: Viviana Casasola, Simone Bianchi, Laura Magrini, Aleksandr V. Mosenkov, Francesco Salvestrini, Maarten Baes, Francesco Calura, Letizia P. Cassarà, Christopher J. R. Clark, Edvige Corbelli, Jacopo Fritz, Frédéric Galliano, Elisabetta Liuzzo, Suzanne Madden, Angelos Nersesian, Francesca Pozzi, Sambit Roychowdhury, Ivano Baronchelli, Matteo Bonato, Carlotta Gruppioni, Lara Pantoni

Publikováno v: Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, 668 (A130), 38p. ⟨10.1051/0004-6361/202245043⟩
ASTRONOMY & ASTROPHYSICS

We perform a homogeneous analysis of an unprecedented set of spatially resolved scaling relations (SRs) between ISM components and other properties in the range of scales 0.3-3.4 kpc. We also study some ratios: dust-to-stellar, dust-to-gas, and dust-

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c091a29aee7acd9f8190151030da8994
http://arxiv.org/abs/2210.15993

Candidate Population III stellar complex at z = 6.629 in the MUSE Deep Lensed Field

Autor: E. Sani, Paolo Tozzi, Mario Nonino, Eros Vanzella, Laura Pentericci, M. Mignoli, Amata Mercurio, Adriano Fontana, Tommaso Treu, G. B. Caminha, Roberto Gilli, Francesco Calura, Andrea Grazian, Massimo Meneghetti, Max Gronke, Piero Rosati, Claudio Grillo, Mark Dijkstra, Karina Caputi, Italo Balestra, G. Cupani, Marco Castellano, Stefano Cristiani

Publikováno v: Monthly Notices of the Royal Astronomical Society: Letters, 494(1), L81-L85

We discovered a strongly lensed (\mu >40) Lya emission at z=6.629 (S/N~18) in the MUSE Deep Lensed Field (MDLF) targeting the Hubble Frontier Field galaxy cluster MACS~J0416. Dedicated lensing simulations imply that the Lya emitting region necessaril

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5737de03b72c1d6eeae01158c8e99b61
https://hdl.handle.net/11370/82754443-2a01-4ccf-af00-5f3f74b27758

A new estimate of the cosmic star formation density from a radio-selected sample, and the contribution of $H$-dark galaxies at $z \geq 3$

Autor: Andrea Enia, Margherita Talia, Francesca Pozzi, Andrea Cimatti, Ivan Delvecchio, Gianni Zamorani, Quirino D’Amato, Laura Bisigello, Carlotta Gruppioni, Giulia Rodighiero, Francesco Calura, Daniele Dallacasa, Marika Giulietti, Luigi Barchiesi, Meriem Behiri, Michael Romano

The Star Formation Rate Density (SFRD) history of the Universe is well constrained up to redshift $z \sim 2$. At earlier cosmic epochs, the picture has been largely inferred from UV-selected galaxies (e.g. Lyman-break galaxies, LBGs). However, LBGs'

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f094bf8f34654d450a251e6a6f1ab24e

The role of Type Ia supernova feedback on the second generation formation in globular clusters

Autor: Elena Lacchin, Francesco Calura, Enrico Vesperini

Very little is known about the physical processes which determined the end of star formation in globular clusters (GC). By means of 3D hydrodynamic simulations, we study for the first time how the formation and the chemical properties of second gener

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::20a76a7ea3f165c33f6948d594ea8fcf