Turnitin
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CARMENES input catalogue of M dwarfs-V. Luminosities, colours, and spectral energy distributions
Context. The relevance of M dwarfs in the search for potentially habitable Earth-sized
planets has grown significantly in the last years. Aims. In our on-going effort to …
planets has grown significantly in the last years. Aims. In our on-going effort to …
Partial Tidal Disruptions of Main-sequence Stars by Intermediate-mass Black Holes
We study close encounters of a 1 M⊙ middle-age main-sequence star (modeled using
MESA) with massive black holes through hydrodynamic simulations, and explore in …
MESA) with massive black holes through hydrodynamic simulations, and explore in …
Wind-reprocessed transients from stellar-mass black hole Tidal Disruption Events
Tidal disruptions of stars by stellar-mass black holes are expected to occur frequently in
dense star clusters. Building upon previous studies that performed hydrodynamic …
dense star clusters. Building upon previous studies that performed hydrodynamic …
Close encounters of star–black hole binaries with single stars
Multibody dynamical interactions of binaries with other objects are one of the main driving
mechanisms for the evolution of star clusters. It is thus important to bring our understanding …
mechanisms for the evolution of star clusters. It is thus important to bring our understanding …
Close encounter of three black holes revisited
We study the evolution of close triple black hole system with full numerical relativity
techniques. We consider an equal mass non spinning hierarchical system with an inner …
techniques. We consider an equal mass non spinning hierarchical system with an inner …
Close encounters of tight binary stars with stellar-mass black holes
Strong dynamical interactions among stars and compact objects are expected in a variety of
astrophysical settings, such as star clusters and the disks of active galactic nuclei. Via a suite …
astrophysical settings, such as star clusters and the disks of active galactic nuclei. Via a suite …
Tidal disruption events from three-body scatterings and eccentricity pum** in the discs of active galactic nuclei
Tidal disruption events (TDEs) are routinely observed in quiescent galaxies, as stars from
the nuclear star cluster are scattered into the loss cone of the central supermassive black …
the nuclear star cluster are scattered into the loss cone of the central supermassive black …
“Tidal Peeling Events”: Low-eccentricity Tidal Disruption of a Star by a Stellar-mass Black Hole
Close encounters between stellar-mass black holes (BHs) and stars occur frequently in
dense star clusters and in the disks of active galactic nuclei. Recent studies have shown that …
dense star clusters and in the disks of active galactic nuclei. Recent studies have shown that …
Close encounters of black hole—star binaries with stellar-mass black holes
Dynamical interactions involving binaries play a crucial role in the evolution of star clusters
and galaxies. We continue our investigation of the hydrodynamics of three-body encounters …
and galaxies. We continue our investigation of the hydrodynamics of three-body encounters …
Multimessenger astronomy with black holes
Most, if not all, galaxies harbor at their center a supermassive black hole (SMBH) that sculpts
the dynamics of objects inhabiting galactic nuclei. SMBH binaries (SMBHBs) are expected to …
the dynamics of objects inhabiting galactic nuclei. SMBH binaries (SMBHBs) are expected to …