Zobrazeno 1 - 9
of 9
pro vyhledávání: '"Andrea Kulier"'
Autor:
Andrea Kulier, Bianca Poggianti, Stephanie Tonnesen, Rory Smith, Alessandro Ignesti, Nina Akerman, Antonino Marasco, Benedetta Vulcani, Alessia Moretti, Anna Wolter
Publikováno v:
The Astrophysical Journal, Vol 954, Iss 2, p 177 (2023)
Ram pressure stripping of satellite galaxies is thought to be a ubiquitous process in galaxy clusters, and a growing number of observations reveal satellites at different stages of stripping. However, in order to determine the fate of any individual
Externí odkaz:
https://doaj.org/article/597e9b3d6bbb463289f32919b22af167
Autor:
Anna S Saburova, Igor V Chilingarian, Andrea Kulier, Gaspar Galaz, Kirill A Grishin, Anastasia V Kasparova, Victoria Toptun, Ivan Yu Katkov
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2023, 520 (1), pp.L85-L90. ⟨10.1093/mnrasl/slad005⟩
Monthly Notices of the Royal Astronomical Society, 2023, 520 (1), pp.L85-L90. ⟨10.1093/mnrasl/slad005⟩
Rare giant low surface brightness galaxies (gLSBGs) act as a stress test for the current galaxy formation paradigm. To answer the question `How rare are they?' we estimate their volume density in the local Universe. A visual inspection of 120~sq.~deg
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::37b3059215ce108a742f4918121d4e28
http://arxiv.org/abs/2209.09906
http://arxiv.org/abs/2209.09906
Autor:
Ariel Werle, Bianca Poggianti, Alessia Moretti, Callum Bellhouse, Benedetta Vulcani, Marco Gullieuszik, Mario Radovich, Jacopo Fritz, Alessandro Ignesti, Johan Richard, Geneviève Soucail, Gustavo Bruzual, Stephane Charlot, Matilde Mingozzi, Cecilia Bacchini, Neven Tomicic, Rory Smith, Andrea Kulier, Giorgia Peluso, Andrea Franchetto
Publikováno v:
The Astrophysical Journal
The Astrophysical Journal, 2022, 930, ⟨10.3847/1538-4357/ac5f06⟩
The Astrophysical Journal, 2022, 930, ⟨10.3847/1538-4357/ac5f06⟩
We present results from MUSE spatially-resolved spectroscopy of 21 post-starburst galaxies in the centers of 8 clusters from $z\sim0.3$ to $z\sim0.4$. We measure spatially resolved star-formation histories (SFHs), the time since quenching ($t_Q$) and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7c0158193184a5f4986da19623c098ec
https://hal-insu.archives-ouvertes.fr/insu-03672016
https://hal-insu.archives-ouvertes.fr/insu-03672016
Autor:
Tom Theuns, Nelson Padilla, E. Paillas, Matthieu Schaller, Robert A. Crain, Joop Schaye, Andrea Kulier, Richard G. Bower
Publikováno v:
Monthly notices of the Royal Astronomical Society, 2019, Vol.482(3), pp.3261-3273 [Peer Reviewed Journal]
Monthly Notices of the RAS (0035-8711), 482(3), 3261-3273
Monthly Notices of the RAS (0035-8711), 482(3), 3261-3273
The EAGLE simulation suite has previously been used to investigate the relationship between the stellar mass of galaxies, $M_{*}$, and the properties of dark matter halos, using the hydrodynamical reference simulation combined with a dark matter only
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c2161316b139197e60076a364c044d44
http://dro.dur.ac.uk/26819/2/26819.pdf
http://dro.dur.ac.uk/26819/2/26819.pdf
Publikováno v:
Monthly Notices of the RAS (0035-8711), 496(3), 3996-4016
We investigate the formation and properties of low surface brightness galaxies (LSBGs) with $M_{*} > 10^{9.5} \mathrm{M_{\odot}}$ in the EAGLE hydrodynamical cosmological simulation. Galaxy surface brightness depends on a combination of stellar mass
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f64d3b02bfb9dca11aa43b03bd18fb0f
https://doi.org/10.48550/arxiv.1910.05345
https://doi.org/10.48550/arxiv.1910.05345
Autor:
Neta A. Bahcall, Andrea Kulier
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 439:2505-2514
How is mass distributed in the Universe? How does it compare with the distribution of light and stars? We address these questions by examining the distribution of mass, determined from weak lensing observations, and starlight, around $>10^5$ SDSS Max
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6f23ff6e2ab0d9a281502255269e13ff
https://doi.org/10.1093/mnras/stu107
https://doi.org/10.1093/mnras/stu107
Autor:
Alison L. Coil, Martin Elvis, Kevin Bundy, Francesca Civano, M. Schramm, Alexie Leauthaud, Andrew J. Benson, Peter Capak, Richard Massey, Andrea Kulier, Andreas Schulze, Jason Rhodes
Publikováno v:
Monthly Notices of the Royal Astronomical Society, vol 446, iss 2
Monthly notices of the Royal Astronomical Society, 2015, Vol.446(2), pp.1874-1888 [Peer Reviewed Journal]
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, vol 446, iss 2
Leauthaud, Alexie; Benson, Andrew J; Civano, Francesca; Coil, Alison L; Bundy, Kevin; Massey, Richard; et al.(2015). The dark matter haloes of moderate luminosity X-ray AGN as determined from weak gravitational lensing and host stellar masses. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 446(2), 1874-1888. doi: 10.1093/mnras/stu2210. UC San Diego: Retrieved from: http://www.escholarship.org/uc/item/3395s37x
Monthly notices of the Royal Astronomical Society, 2015, Vol.446(2), pp.1874-1888 [Peer Reviewed Journal]
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, vol 446, iss 2
Leauthaud, Alexie; Benson, Andrew J; Civano, Francesca; Coil, Alison L; Bundy, Kevin; Massey, Richard; et al.(2015). The dark matter haloes of moderate luminosity X-ray AGN as determined from weak gravitational lensing and host stellar masses. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 446(2), 1874-1888. doi: 10.1093/mnras/stu2210. UC San Diego: Retrieved from: http://www.escholarship.org/uc/item/3395s37x
Understanding the relationship between galaxies hosting active galactic nuclei (AGN) and the dark matter halos in which they reside is key to constraining how black-hole fueling is triggered and regulated. Previous efforts have relied on simple halo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::dc27534ac39b989b500b1239e5b9ce88
https://escholarship.org/uc/item/3395s37x
https://escholarship.org/uc/item/3395s37x
Autor:
Jeremiah P. Ostriker, Andrea Kulier
Halo Abundance Matching has been used to construct a one-parameter mapping between galaxies and dark matter haloes by assuming that halo mass and galaxy luminosity (or stellar mass) are monotonically related. While this approach has been reasonably s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e2ec892aad428b25a17edabcdbaef15b
Publikováno v:
The Astrophysical Journal. 799:178
Accretion is thought to primarily contribute to the mass accumulation history of supermassive black holes throughout cosmic time. While this may be true at high redshifts, at lower redshifts and for the most massive black holes mergers themselves mig
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::62a97522bec4bf91e674b34ec63b2f67
https://doi.org/10.1088/0004-637x/799/2/178
https://doi.org/10.1088/0004-637x/799/2/178