activity
20202025
most citedConstraining the origin of the planetary debris surrounding ZTF J0139+5245 through rotational fission of a triaxial asteroid

31 citations · 82 across the 6 of their papers we have counts for

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Showing astro-ph.EPShow all

7 papers · 1 filter

astro-ph.EP2025★ 13 cited

Tracing the formation and migration history: molecular signatures in the atmosphere of misaligned hot Jupiter WASP-94Ab using JWST NIRSpec/G395H

Eva-Maria Ahrer, Siddharth Gandhi, Lili Alderson +12

The discovery of hot Jupiters that orbit very close to their host stars has long challenged traditional models of planetary formation and migration. Characterising their atmospheri…

astro-ph.EP2024

Atmospheric characterisation and tighter constraints on the orbital misalignment of WASP-94 A b with HARPS

E. Ahrer, J. V. Seidel, L. Doyle +10

We present high spectral resolution observations of the hot Jupiter WASP-94 A b using the HARPS instrument on ESO's 3.6m telescope in La Silla, Chile. We probed for Na absorption i…

astro-ph.EP2023★ 5 cited

Binary asteroid scattering around white dwarfs

Catriona H. McDonald, Dimitri Veras

Increasing observations of white dwarf atmospheric pollution and disrupting planetesimals is driving increased studies into the fate of exo-asteroids around post-main-sequence star…

astro-ph.EP2021★ 15 cited

White dwarf planetary debris dependence on physical structure distributions within asteroid belts

Catriona H. McDonald, Dimitri Veras

White dwarfs which exhibit transit signatures of planetary debris and accreted planetary material provide exceptional opportunities to probe the material composition and dynamical…

astro-ph.EP2020

Linking the formation and fate of exo-Kuiper belts within solar system analogues

Dimitri Veras, Katja Reichert, Francesco Flammini Dotti +7

Escalating observations of exo-minor planets and their destroyed remnants both passing through the solar system and within white dwarf planetary systems motivate an understanding o…

astro-ph.EP2020★ 18 cited

Constraining planet formation around 6-8 stars

Dimitri Veras, Pier-Emmanuel Tremblay, J. J. Hermes +4

Identifying planets around O-type and B-type stars is inherently difficult; the most massive known planet host has a mass of only about . However, planetary systems whi…