activity
20232025
collaborators

6 papers

astro-ph.GA2025

Chandra Rules Out Super-Eddington Accretion Models For Little Red Dots

Andrea Sacchi, Akos Bogdan

One of the most puzzling discoveries by JWST is the population of high-redshift, red, and compact galaxies dubbed little red dots (LRDs). Based on broad-line diagnostics, these gal…

astro-ph.HE2025

Probing the interstellar medium toward GRB 221009A through X-ray dust scattering

B. Vaia, Ž. Bošnjak, A. Bracco +5

The observation of 21 X-ray dust-scattering rings around the extraordinarily bright gamma-ray burst (GRB) 221009A provides a unique opportunity to study the interstellar medium (IS…

astro-ph.HE2025

Hyperluminous Supersoft X-Ray Sources in the Chandra Catalog

Andrea Sacchi, Kevin Paggeot, Steven Dillmann +2

Hyperluminous supersoft X-ray sources, such as bright extragalactic sources characterized by particularly soft X-ray spectra, offer a unique opportunity to study accretion onto sup…

astro-ph.GA2025

Detection of Anisotropies in the Circumgalactic Medium of Disk Galaxies: Supermassive Black Hole Activity or Star Formation-driven Outflows?

Andrea Sacchi, Akos Bogdan, Nhut Truong

Gamma and X-ray observatories have revealed spectacular structures in the emission of the tenuous hot gas surrounding the Milky Way (MW), known as the Fermi and eROSITA bubbles. Ga…

astro-ph.SR2024

The impact of periastron passage on the X-ray and optical properties of the Symbiotic System R Aquarii

D. A. Vásquez-Torres, J. A. Toalá, A. Sacchi +4

Multi-epoch Chandra and XMM-Newton observations of the symbiotic system R Aquarii (R Aqr) spanning 22 yr are analysed by means of a reflection model produced by an accretion disc.…

astro-ph.HE2023

A soft and transient ultraluminous X-ray source with 6-h modulation in the NGC 300 galaxy

A. Sacchi, P. Esposito, D. de Martino +13

We investigate the nature of CXOU J005440.5-374320 (J0054), a peculiar bright ( erg/s) and soft X-ray transient in the spiral galaxy NGC 300 with a 6-hour per…