F
Filippo Fraternali
Researcher at Kapteyn Astronomical Institute
Publications - 248
Citations - 11524
Filippo Fraternali is an academic researcher from Kapteyn Astronomical Institute. The author has contributed to research in topics: Galaxy & Star formation. The author has an hindex of 56, co-authored 239 publications receiving 9883 citations. Previous affiliations of Filippo Fraternali include INAF & University of Oxford.
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Cold gas accretion in galaxies
TL;DR: In this article, it was shown that a large fraction of this gas is generated by galactic fountains, while a large part of it is likely to be of extragalactic origin, and the Milky Way has extra-planar gas complexes: the Intermediate and High Velocity Clouds (IVCs and HVCs).
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Cold gas accretion in galaxies
TL;DR: In this article, it was shown that in order to reach the accretion rates needed to sustain the observed star formation, additional infall of large amounts of gas from the intergalactic medium (IGM) seems to be required.
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The Cold Gaseous Halo of NGC 891
TL;DR: In this article, H I observations of the edge-on galaxy NGC 891 were performed and revealed a huge gaseous halo, much more extended than seen previously and containing almost 30% of the H I.
Advancing Astrophysics with the Square Kilometre Array
S. L. Blyth,van der Thijs Hulst,Marc Verheijen,Barbara Catinella,Filippo Fraternali,Martha P. Haynes,Kelley M. Hess,Baerbel Koribalski,Claudia del P. Lagos,Martin Meyer,Danail Obreschkow,Attila Popping,Chris Power,Lourdes Verdes-Montenegro,Martin Zwaan +14 more
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3D BAROLO: a new 3D algorithm to derive rotation curves of galaxies
TL;DR: In this article, the authors present a new code that derives rotation curves of galaxies from emission-line observations, fitting 3D tilted-ring models to spectroscopic data cubes and can be used with a variety of observations: from H I and molecular lines to optical recombination lines.