118 citations · 719 across the 34 of their papers we have counts for
36 papers
Effect of Neutron Star Jets on Common Envelope Evolution
Deepanshu Gurjar, Luke Chamandy, Eric G. Blackman +3
The common envelope (CE) phase is a key stage in binary star evolution that is still not very well understood. Once engulfed by the giant star, the binary companion may accrete env…
Radio Continuum Emission from Evolving Star-Forming Galaxies -- I. Correlations Involving the Total Synchrotron Luminosity
Sukanta Ghosh, Luke Chamandy, Charles Jose +3
Synchrotron radiation dominates the continuum emission of star-forming galaxies in the frequency range from a few to about . We model the total synchrotron…
Understanding the Drag Torque in Common Envelope Evolution
Soumik Bhattacharyya, Luke Chamandy, Eric G. Blackman +2
Common envelope (CE) evolution is largely governed by the drag torque applied on the in-spiralling stellar components by the envelope. Previous work has shown that idealized models…
The fine structure of the mean magnetic field in M31
Indrajit Paul, R. Vasanth Kashyap, Tuhin Ghosh +4
To explore the spatial variations of the regular (mean) magnetic field of the Andromeda galaxy (M31), we use Fourier analysis in azimuthal angle along four rings in the galaxy's pl…
Galactic magnetic fields II. Applying the model to nearby galaxies
Rion Glenn Nazareth, Gayathri Santhosh, Luke Chamandy
Many spiral galaxies host magnetic fields with energy densities comparable to those of the turbulent and thermal motions of their interstellar gas. However, quantitative comparison…
Second-generation planet formation after tidal disruption from common envelope evolution
Luke Chamandy, Jason Nordhaus, Eric G. Blackman +1
We propose that certain white dwarf (WD) planets, such as WD 1856+534 b, may form out of material from a stellar companion that tidally disrupts from common envelope evolution with…