Mid-infrared sizes of circumstellar disks around Herbig Ae/Be stars measured with MIDI on the VLTI

By C. Leinert, R. van Boekel, L. Waters, O. Chesneau, F. Malbet, R. Köhler, W. Jaffe, T. Ratzka, A. Dutrey, T. Preibisch and 28 more. 2004

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Star and Protoplanetary Disk Properties in Orion's Suburbs (2009, background): “…reproduce the SEDs of young stars, and observations that spatially resolve these objects confirm that interpretation (e.g. Eisner et al. 2003; Leinert et al. 2004; Monnieret al. 2005; Akeson et al. 2005a,b; Isella et al. 2006; Monnier et al. 2006; Eisner et al. 2007; Acke et al. 2008; Kraus…”
STRUCTURES IN THE PROTOPLANETARY DISK OF HD142527 SEEN IN POLARIZED SCATTERED LIGHT (2013, background): “The inner disk is highly crystalline and is responsible for the mid-infrared emission (Leinert et al. 2004; van Boekel et al. 2005).”
Accretion disks in luminous young stellar objects (2015, methodology): “This SED based idea is found to be consistent with resolved observations using mid-IR interferometry (Leinert et al. 2004, Di Folco et al. 2009).”
The warm gas atmosphere of the HD 100546 disk seen by Herschel - Evidence of a gas-rich, carbon-poor atmosphere? (2012, background): “Interferometric observations (VLT-AMBER and MIDI, Leinert et al. 2004; Petrov et al. 2007) confirm the presence of the inner hole directly and set rhole ∼ 13 AU (Benisty et al. 2010).”