Posted in astro-ph.EP · 2026-01-17 · Brianna Zawadzki, Anna Fehr, A. Meredith Hughes, Elias Mansell, Jamar Kittling, Yinuo Han, Catherine Hou, Margaret Pan, Julien Milli, Johan Olofsson, Tim D. Pearce, Antranik A. Sefilian, Aliya Nurmohamed, Junu Lee, Yamani Mpofu, Myriam Bonduelle, Mark Booth, Aoife Brennan, Carlos del Burgo, John M. Carpenter, Gianni Cataldi, Eugene Chiang, Steve Ertel, Thomas Henning, Marija R. Jankovic, Grant M. Kennedy, Ágnes Kóspál, Alexander V. Krivov, Joshua B. Lovell, Patricia Luppe, Meredith A. MacGregor, Sorcha Mac Manamon, Sebastian Marino, Jonathan P. Marshall, Luca Matrà, Attila Moór, Sebastián Pérez, Philipp Weber, David J. Wilner, Mark C. Wyatt
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 ${\gtrsim}10$ Myr old. Millimeter-wavelength observations are particularly important, as the grains probed by these observations are not strongly affected by...