Area of research
Astronomy and Astrophysics
Research interest
Research interests include Physics, Astrophysics, Astronomy, Supermassive black hole, Galaxy, and Black hole (networking).
Growth of massive black holes in FFB galaxies at cosmic dawn
Disruptions of stars and binary systems on chaotic orbits in an axisymmetric Milky Way centre
Late-time Evolution of Magnetized Disks in Tidal Disruption Events
Fragmentation in collapsar discs: migration, growth, and emission
ULTRASAT: A Wide-field Time-domain UV Space Telescope
Stream–disk shocks as the origins of peak light in tidal disruption events
The effect of thermal torques on AGN disc migration traps and gravitational wave populations
AT2018fyk: Candidate Tidal Disruption Event by a (Super)Massive Black Hole Binary
Tidal Disruption Event AT2020ocn: Early Time X-Ray Flares Caused by a Possible Disk Alignment Process
Heating galaxy clusters with interacting dark matter
Counting the Unseen. I. Nuclear Density Scaling Relations for Nucleated Galaxies
Magnetically dominated discs in tidal disruption events and quasi-periodic eruptions
The growth of intermediate mass black holes through tidal captures and tidal disruption events
XMM-<i>Newton</i>-discovered Fast X-ray Transients: host galaxies and limits on contemporaneous detections of optical counterparts
Optical/UV emission in the Tidal Disruption Event ASASSN-14li: implications of disc modelling
A Census of Archival X-Ray Spectra for Modeling Tidal Disruption Events
Interacting Stellar EMRIs as Sources of Quasi-periodic Eruptions in Galactic Nuclei
Feedback-dominated Accretion Flows
The scientific payload of the Ultraviolet Transient Astronomy Satellite (ULTRASAT)
A Library of Synthetic X-Ray Spectra for Fitting Tidal Disruption Events
The rapidly spinning intermediate-mass black hole 3XMM J150052.0+015452
Density wakes driving dynamical friction in cored potentials
The thermodynamics of stellar multiplicity: an analytic model for the dynamical evolution of binary star populations in dense stellar environments due to single–binary interactions
Revisiting stellar orbits and the Sgr <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msup><mml:mrow><mml:mi mathvariant="normal">A</mml:mi></mml:mrow><mml:mrow><mml:mo>*</mml:mo></mml:mrow></mml:msup></mml:mrow></mml:math> quadrupole moment
Tidal disruption discs formed and fed by stream–stream and stream–disc interactions in global GRHD simulations
The Process of Stellar Tidal Disruption by Supermassive Black Holes
The Observed Mass Distribution of Galactic Black Hole LMXBs Is Biased against Massive Black Holes
Editorial to the Topical Collection: The Tidal Disruption of Stars by Massive Black Holes
Intermediate mass black hole formation in compact young massive star clusters