activity
20172023
most citedDo instabilities in high-multiplicity systems explain the existence of close-in white dwarf planets?

35 citations · 106 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR20231 cited

Synthetic X-ray emission from white dwarf accreting planetary material

S. Estrada-Dorado, V. Lora, J. A. Toalá +4

The emission of hard X-rays associated with white dwarfs (WD) can be generated by the presence of a stellar companion either by the companion's coronal emission or by an accretion…

astro-ph.EP202211 cited

Disentangling the parameter space: The role of planet multiplicity in triggering dynamical instabilities on planetary systems around white dwarfs

R. F. Maldonado, E. Villaver, A. J. Mustill +1

Planets orbiting intermediate and low-mass stars are in jeopardy as their stellar hosts evolve to white dwarfs (WDs) because the dynamics of the planetary system changes due to the…

astro-ph.EP202035 cited

Do instabilities in high-multiplicity systems explain the existence of close-in white dwarf planets?

R. F. Maldonado, E. Villaver, A. J. Mustill +2

We investigate the origin of close-in planets and related phenomena orbiting white dwarfs (WDs), which are thought to originate from orbits more distant from the star. We use the p…

astro-ph.EP202031 cited

Understanding the origin of white dwarf atmospheric pollution by dynamical simulations based on detected three-planet systems

R. F. Maldonado, E. Villaver, A. J. Mustill +2

Between 25-50 % of white dwarfs (WD) present atmospheric pollution by metals, mainly by rocky material, which has been detected as gas/dust discs, or in the form of photometric tra…

astro-ph.EP202023 cited

Dynamical evolution of two-planet systems and its connection with white dwarf atmospheric pollution

R. F. Maldonado, E. Villaver, A. J. Mustill +2

Asteroid material is detected in white dwarfs (WDs) as atmospheric pollution by metals, in the form of gas/dust discs, or in photometric transits. Within the current paradigm, mino…

astro-ph.SR20175 cited

Infrared excesses in stars with and without planets using revised photometry

Raul F. Maldonado, Miguel Chavez, Emanuele Bertone +1

We present an analysis on the potential prevalence of mid infrared excesses in stars with and without planetary companions. Based on an extended database of stars detected with the…