Zobrazeno 1 - 10
of 177
pro vyhledávání: '"Andrea V Macciò"'
Autor:
Dhurba Tripathi, Paolo Giommi, Adriano Di Giovanni, Rawdha R. Almansoori, Nouf Al Hamly, Francesco Arneodo, Andrea V. Macciò, Goffredo Puccetti, Ulisses Barres de Almeida, Carlos Brandt, Simonetta Di Pippo, Michele Doro, Davit Israyelyan, A. M. T. Pollock, Narek Sahakyan
Publikováno v:
The Astronomical Journal, Vol 167, Iss 3, p 116 (2024)
Firmamento ( https://firmamento.hosting.nyu.edu ) is a new-concept, web-based, and mobile-friendly data analysis tool dedicated to multifrequency/multimessenger emitters, as exemplified by blazars. Although initially intended to support a citizen res
Externí odkaz:
https://doaj.org/article/8b5a188537304ff4a6656e13fe7d863e
Publikováno v:
The Astrophysical Journal, Vol 961, Iss 1, p 144 (2024)
Externí odkaz:
https://doaj.org/article/5382e3785db449f1b1f87ee8193cd398
Publikováno v:
The Astrophysical Journal, Vol 957, Iss 1, p 7 (2023)
We present simulated galaxy spectral energy distributions (SEDs) from the far-ultraviolet (FUV) through the far-infrared (FIR), created using hydrodynamic simulations and radiative transfer calculations, suitable for the validation of SED modeling te
Externí odkaz:
https://doaj.org/article/6730def34a6e46c580b1b101354817a4
We present a catalogue of dynamical properties for 2368 late-type galaxies from the MaNGA survey. The latter complements the catalogue of photometric properties for the same sample based on deep optical DESI photometry processed with AutoProf. Rotati
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a03760233bdf09eaf88fb6ebf553476b
Autor:
Sven Buder, Tobias Buck, Christoph Pfrommer, Jan Rybizki, Andrea V. Macciò, Aura Obreja, Matthias Steinmetz, Melissa Ness
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 508:3365-3387
With the advent of large spectroscopic surveys the amount of high quality chemo-dynamical data in the Milky Way (MW) increased tremendously. Accurately and correctly capturing and explaining the detailed features in the high-quality observational dat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::232b2ae2ba6b092bb306877c625e6e2d
https://doi.org/10.1093/mnras/stab2736
https://doi.org/10.1093/mnras/stab2736
An extensive catalog of spatially-resolved galaxy rotation curves and multi-band optical light profiles for 1752 observed spiral galaxies is assembled to explore the drivers of diversity in galaxy structural parameters, rotation curve shapes, and ste
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::10986d37151a183fd38cde8c36caec1b
http://arxiv.org/abs/2204.02412
http://arxiv.org/abs/2204.02412
Autor:
Andrea V Macciò, Mohamad Ali-Dib, Pavle Vulanovic, Hind Al Noori, Fabian Walter, Nico Krieger, Tobias Buck
Cosmological galaxy formation simulations are still limited by their spatial/mass resolution and cannot model from first principles some of the processes, like star formation, that are key in driving galaxy evolution. As a consequence they still rely
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d8deb81ca734f83c4dc23772dd7f45a3
Autor:
Stefan Waterval, Sana Elgamal, Matteo Nori, Mario Pasquato, Andrea V Macciò, Marvin Blank, Keri L Dixon, Xi Kang, Tengiz Ibrayev
Although active galactic nuclei (AGN) feedback is required in simulations of galaxies to regulate star formation, further downstream effects on the dark matter distribution of the halo and stellar kinematics of the central galaxy can be expected. We
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::dc33df1348d4508f104fe6c4c820da04
The transition of high-mass galaxies from being blue and star forming to being red and dead is a crucial step in galaxy evolution, yet not fully understood. In this work, we use the NIHAO suite of galaxy simulations to investigate the relation betwee
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c51e0eac224f8c51574ca3781d980be5
We present the first high-resolution zoom-in simulation of a Milky-way-like halo extracted from the Aquarius Project in the Fuzzy Dark Matter (FDM) framework. We use the N-body code AX-GADGET, based on a particle oriented solution of the Schr\"{o}din
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f63fd8a297ad30375c980097e2bec127