E
Enrico Maria Corsini
Researcher at University of Padua
Publications - 109
Citations - 3117
Enrico Maria Corsini is an academic researcher from University of Padua. The author has contributed to research in topics: Galaxy & Bulge. The author has an hindex of 29, co-authored 109 publications receiving 2815 citations. Previous affiliations of Enrico Maria Corsini include Max Planck Society & INAF.
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Journal ArticleDOI
The population of barred galaxies in the local universe - I. Detection and characterisation of bars
J. A. L. Aguerri,Jairo Méndez-Abreu,Jairo Méndez-Abreu,Jairo Méndez-Abreu,Enrico Maria Corsini +4 more
TL;DR: In this paper, a volume-limited sample of 2106 disc galaxies was studied to derive the bar fraction, length, and strength as a function of the morphology, size, local galaxy density, light concentration, and color of the host galaxy.
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On the correlations between galaxy properties and supermassive black hole mass
TL;DR: In this paper, a large sample of upper limits and accurate estimates of supermassive black hole (SMBH) masses coupled with libraries of host galaxy velocity dispersions, rotational velocities and photometric parameters extracted from the Sloan Digital Sky Survey (SDSS) i-band images were used to establish correlations between the SMBH and host galaxy parameters.
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Dynamical modelling of luminous and dark matter in 17 Coma early-type galaxies
Jens Thomas,Roberto P. Saglia,Ralf Bender,Daniel Thomas,Karl Gebhardt,John Magorrian,Enrico Maria Corsini,Gary Wegner +7 more
TL;DR: In this article, the authors used Axisymmetric Schwarzschild models to derive stellar mass-tolight ratios and dark halo parameters for 17 early-type galaxies in the Coma cluster.
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Measurement of fast bars in a sample of early‐type barred galaxies
TL;DR: In this paper, surface photometry and stellar kinematics of a sample of five SB0 galaxies: ESO 139-G009, IC 874, NGC 1308, and NGC 1440, were measured using the Tremaine-Weinberg method.
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A fast bar in the post-interaction galaxy NGC 1023
TL;DR: In this article, Knapen et al. measured the bar pattern speed of the SB0 galaxy NGC 1023 using the Tremaine-Weinberg (1984) method with stellar-absorption slit spectroscopy.