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Eccentric neutron star disk driven type II outburst pairs in Be/X-ray binaries
Alessia Franchini, Rebecca G. Martin
Be star X-ray binaries are transient systems that show two different types of outbursts. Type I outbursts occur each orbital period while type II outbursts have a period and durati…
Non-periodic type I Be/X-ray binary outbursts
Rebecca G. Martin, Alessia Franchini
Type I Be/X-ray binary outbursts are driven by mass transfer from a Be star decretion disc to a neutron star companion during each orbital period. Treiber et al. (2021) recently ob…
The competing effect of gas and stars in massive black hole binaries evolution
Elisa Bortolas, Alessia Franchini, Matteo Bonetti +1
Massive black hole binaries are predicted to form during the hierarchical assembly of cosmic structures and will represent the loudest sources of low-frequency gravitational waves…
Circumbinary disc self-gravity governing supermassive black hole binary mergers
Alessia Franchini, Alberto Sesana, Massimo Dotti
Understanding the interaction of massive black hole binaries with their gaseous environment is crucial since at sub-parsec scales the binary is too wide for gravitational wave emis…