{"id":69,"date":"2014-10-06T04:39:40","date_gmt":"2014-10-06T04:39:40","guid":{"rendered":"http:\/\/distantearths.com\/Ilaria\/?page_id=69"},"modified":"2025-06-13T20:30:54","modified_gmt":"2025-06-13T20:30:54","slug":"advising","status":"publish","type":"page","link":"http:\/\/distantearths.com\/Ilaria\/advising\/","title":{"rendered":"Advising"},"content":{"rendered":"

Postdoctoral Fellows:<\/em><\/strong><\/p>\n

\u2013 F. Long (2022-2025, LPL, The University of Arizona). Disk structures and chemistry. 1. The First JWST View of a 30-Myr-old Protoplanetary Disk Reveals a Late-stage Carbon-rich Phase<\/a><\/p>\n

\u2013 M. Fang (2017-2019, LPL, The University of Arizona). Disk Winds. 1. A New Look at T Tauri Star Forbidden Lines: MHD-driven Winds from the Inner Disk<\/a>\u00a0\u2013 2. Double-peaked [O I] Profile: A Likely Signature of the Gaseous Ring around KH 15D<\/a> \u2013 3. A High-resolution Optical Survey of Upper Sco: Evidence for Coevolution of Accretion and Disk Winds<\/a><\/p>\n

\u2013 A. Banzatti (2016-2019, LPL, The University of Arizona). The evolution and dispersal of gas in the planet-forming region of disks. 1. Kinematic Links and the Coevolution of MHD Winds, Jets, and Inner Disks<\/a> \u2013 2. Hints for Icy Pebble Migration Feeding an Oxygen-rich Chemistry in the Inner Planet-forming Region of Disks<\/a><\/p>\n

\u2013 G. Mulders (2013-2018, LPL, The University of Arizona), Kepler exoplanets and planet formation. 1.\u00a0 A stellar-mass-dependent drop in planet occurrence rates<\/a>\u00a0<\/a>\u2013 2. The Snow Line in Viscous Disks around Low-mass Stars<\/a> \u2013 3. An Increase in the Mass of Planetary Systems around Lower-mass Stars<\/a> \u2013 4. A Super-Solar Metallicity For Stars With Hot Rocky Exoplanets<\/a> \u2013 5.Constraints from Dust Mass and Mass Accretion Rate Measurements on Angular Momentum Transport in Protoplanetary Disks<\/a> \u2013 6. The Exoplanet Population Observation Simulator<\/a><\/p>\n

\u2013 E. Rigliaco (2011-2014, LPL, The University of Arizona), Disk evolution and dispersal. 1. \u00a0 Understanding the Origin of the [O I] Low-velocity Component from T Tauri Stars<\/a> \u2013 2. Extending Accretion Diagnostics to the Mid-Infrared Wavelengths<\/a><\/p>\n

\u2013 D. Fedele (2010-2011, Johns Hopkins University), Disk chemistry. 1.Water Depletion in the Disk Atmosphere of Herbig AeBe Stars<\/a> \u2013 2. On the Asymmetry of the OH Ro-vibrational Lines in HD 100546<\/a><\/p>\n

\u2013 V. Roccatagliata (2010-2011, Space Telescope Science Institute), Re-reduction of archival Spitzer\/IRS low-resolution spectra, some data included in\u00a0 The protoplanetary disk of FT Tauri: multiwavelength data analysis and modeling<\/a><\/p>\n

\u2013 B. Riaz (2010-2011, Space Telescope Science Institute), Disk structure.\u00a0 The unusual protoplanetary disk around the T Tauri star ET Chamaeleontis<\/a><\/p>\n

Graduate students:<\/strong><\/em><\/p>\n

\u2013 N. Bajaj, PhD (2022-pres, LPL, The University of Arizona), Disk Winds. 1. JWST MIRI MRS Observations of T Cha: Discovery of a Spatially Resolved Disk Wind<\/a>\u2013 2. Class I\/II Jets with JWST: Mass-loss Rates, Asymmetries, and Binary-induced Wigglings<\/a><\/p>\n

\u2013 C. Xie, PhD (2022-pres, LPL, The University of Arizona), Protoplanetary Disks. 1. Water-rich Disks around Late M Stars Unveiled: Exploring the Remarkable Case of Sz 114<\/a>\u2013 2. JWST Captures a Sudden Stellar Outburst and Inner Disk Wall Destruction<\/a><\/p>\n