Showing 1–20 of 48 results
/ Date/ Name
Dec 8, 2006Warm Gas in the Inner Disks around Young Intermediate Mass StarsJul 24, 2023Ro-vibrational Spectroscopy of CI Tau -- Evidence of a Multi-Component Eccentric Disk Induced by a PlanetOct 2, 2007Post-Outburst Observations of V1647 Ori: Detection of a Brief Warm, Molecular OutflowApr 10, 2007Infrared High-Resolution Spectroscopy of Post-AGB Circumstellar Disks. I. HR 4049 - The Winnowing Flow Observed?Aug 2, 2016A Study of Ro-vibrational OH Emission from Herbig Ae/Be StarsJan 3, 2023Herbig Stars: A Quarter Century of ProgressFeb 27, 2026${}^{12}$CO Ro-vibrational Spectroscopy of AB Aurigae -- A Potential Point Source is PresentJul 1, 2009Tracing the inner edge of the disk around HD 100546 with Ro-vibrational CO Emission LinesMar 26, 2020The Planetary Luminosity Problem: "Missing Planets" and the Observational Consequences of Episodic AccretionNov 22, 2013High-Resolution Near Infrared Spectroscopy of HD 100546: II. Analysis of variable rovibrational CO emission linesMar 10, 2015Near Infrared High Resolution Spectroscopy and Spectro-astrometry of Gas in Disks around Herbig Ae/Be StarsSep 2, 2014NIR Spectroscopy of the HAeBe Star HD 100546: III. Further Evidence of an Orbiting Companion?Dec 1, 2025Evolution of the Accretion Rate of Young Intermediate Mass Stars: Implications for Disk Evolution and Planet FormationDec 28, 2023Spectroastrometric Survey of Protoplanetary Disks with Inner Dust CavitiesMay 7, 2018Spectroastrometric Study of Ro-vibrational CO Emission from the Herbig Ae star HD~179218 with iSHELL on the NASA Infrared Telescope FacilityJul 31, 2019High-Resolution Near Infrared Spectroscopy of HD~100546: IV. Orbiting Companion Disappears on ScheduleDec 7, 2017Clarifying the Status of HD 100546 as Observed by the Gemini Planet ImagerSep 19, 2013Gas lines from the 5-Myr old optically thin disk around HD141569A. Herschel observations and modelingDec 12, 2025JWST/NIRSpec Detects Warm CO Emission in the Terrestrial-Planet Zone of HD 131488Dec 14, 2023Vertical Structure of Gas and Dust in Four Debris Disks