activity
19932025
most citedThe X-ray and Radio Connection in Low-luminosity Active Nuclei

153 citations · 2.2k across the 73 of their papers we have counts for

collaborators

73 papers

astro-ph.GA2025

X-ray Halos of Early-Type Galaxies with AGN Feedback and Accretion from a Circumgalactic Medium: models and observations

Silvia Pellegrini, Luca Ciotti, Zhaoming Gan +2

The knowledge of the X-ray properties of the hot gas halos of early-type galaxies has significantly advanced in the past years, for large and homogeneously investigated samples. We…

astro-ph.GA2022★ 7 cited

The Hot Interstellar Medium

Emanuele Nardini, Dong-Woo Kim, Silvia Pellegrini

The interstellar medium (ISM) of galaxies very often contains a gas component that reaches the temperature of several million degrees, whose physical and chemical properties can be…

astro-ph.GA2022

A Parameter Space Exploration of High Resolution Numerically Evolved Early Type Galaxies Including AGN Feedback and Accurate Dynamical Treatment of Stellar Orbits

Luca Ciotti, Jeremiah P. Ostriker, Zhaoming Gan +4

An extensive exploration of the model parameter space of axisymmetric Early-Type Galaxies (ETGs) hosting a central supermassive Black Hole (SMBH) is conducted by means of high reso…

astro-ph.GA2021★ 5 cited

Jeans modeling of axisymmetric galaxies with multiple stellar populations

C. Caravita, L. Ciotti, S. Pellegrini

We present the theoretical framework to efficiently solve the Jeans equations for multi-component axisymmetric stellar systems, focusing on the scaling of all quantities entering t…

astro-ph.HE2020★ 71 cited

Jet collimation in NGC 315 and other nearby AGN

B. Boccardi, M. Perucho, C. Casadio +14

Aims. The collimation of relativistic jets in galaxies is a poorly understood process. Detailed radio studies of the jet collimation region have been performed so far in few indivi…

astro-ph.GA2020★ 6 cited

Two-component galaxy models with a central BH -- II. The ellipsoidal case

L. Ciotti, A. Mancino, S. Pellegrini +1

Recently, two-component spherical galaxy models have been presented, where the stellar profile is described by a Jaffe law, and the total density by another Jaffe law, or by an $r^…