From the 1 of 19 linked papers with an AI index.
19 papers
An Inclined, Eccentric Planet and an Inner Debris Disk Could Reproduce AU Mic Structure
Arcelia Hermosillo Ruiz, Ruth Murray-Clay, Meredith A. MacGregor +1
The authors model how an inclined, eccentric planet interacting with AU Mic's outer debris disk and stellar wind can periodically launch dust clumps that match the observed moving…
A radially broad collisional cascade in the debris disk of Ophiuchi observed by JWST
Yinuo Han, Mark Wyatt, Kate Y. L. Su +13
The A1V star Oph, at a distance of 29.7 pc, is known from Spitzer imaging to host a debris disk with a large radial extent and from its spectral energy distribution to host in…
Revisiting the ultraviolet spectroscopy of the eta Tel edge-on debris disk
Allison Youngblood, Alexis Brandeker, Sebastian Perez +4
We revisit the ultraviolet absorption spectroscopy of the edge-on debris disk surrounding the A0V star Telescopii. Previous work found absorption components at four velocities…
The ALMA survey to Resolve exoKuiper belt Substructures (ARKS) II. The radial structure of debris discs
Yinuo Han, Elias Mansell, Jeff Jennings +38
The ALMA survey to Resolve exoKuiper belt Substructures (ARKS) was recently completed to cover the lack of high-resolution observations of debris discs and to investigate the preva…
The ALMA survey to Resolve exoKuiper belt Substructures (ARKS) V: Comparison between scattered light and thermal emission
J. Milli, J. Olofsson, M. Bonduelle +33
Debris discs are analogues to our own Kuiper belt around main-sequence stars and are therefore referred to as exoKuiper belts. They have been resolved at high angular resolution at…
The ALMA survey to Resolve exoKuiper belt Substructures (ARKS) III: The vertical structure of debris disks
Brianna Zawadzki, Anna Fehr, A. Meredith Hughes +37
Debris disks -- collisionally sustained belts of dust and sometimes gas around main sequence stars -- are remnants of planet formation processes and are found in systems ${\gtrsim}…