Grain growth in the inner regions of Herbig Ae/Be star disks

By R. van Boekel, L. Waters, C. Dominik, J. Bouwman, A. D. Koter, C. Dullemond, F. Paresce. 2003

141 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/0917fc34278b7c1e437b01f8631995f6c8618dc0

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In Astronomy and Astrophysics

Citations in the corpus

The photodissociation and chemistry of CO isotopologues: applications to interstellar clouds and circumstellar disks (2009, background): “Grain growth is an inevitable step towards planet formation and is indeed known to occur in disks (van Boekel et al. 2003; Przygodda et al. 2003; Lommen et al. 2007).”
c2d Spitzer IRS Spectra of Disks around T Tauri Stars. I. Silicate Emission and Grain Growth (2005, methodology): “In contrast, growth of amorphous olivines can mimic the effects of crystallineamorphous silicate mixtures, resulting in weaker, ‘‘flat-topped’’ 10 m silicate features, with similar flux at 9.8 and 11.3 m (e.g., van Boekel et al. 2003; Przygodda et al. 2003; KesslerSilacci et al. 2005).”
Mid-infrared sizes of circumstellar disks around Herbig Ae/Be stars measured with MIDI on the VLTI (2004, background): “HD 144432 The 10 µm silicate band of HD 144432 is one of the strongest observed in HAe stars (van Boekel et al. 2003) and has a shape that closely resembles that of the interstellar medium.”
Gas- and dust evolution in protoplanetary disks (2010, methodology): “Both laboratory experiments (Blum et al. 2000) and observations of the 10µm spectral region (Bouwman et al. 2001; van Boekel et al. 2003) conclude that grain growth must take place in circumstellar disks.”
[O I] 6300 Å emission in Herbig Ae/Be systems: Signature of Keplerian rotation (2005, methodology): “Classification diagram, based on van Boekel et al. (2003).”
Size-sorting dust grains in the surface layers of protoplanetary disks (2008, unknown): “…have been studied in great detail with the Infrared Space Observatory (ISO; e.g. Meeus et al. 2001; Bouwman 2001), with ground-based instruments (van Boekel et al. 2003; Honda et al. 2003) and with the Spitzer Space Telescope (e.g. Apai et al. 2005; Kessler-Silacci et al. 2006; Furlan et al. 2006).”
Multiwavelength analysis for interferometric (sub-)mm observations of protoplanetary disks - Radial constraints on the dust properties and the disk structure (2015, background): “Optical, near-infrared, and mid-infrared observations show evidence of micron-sized dust grains in protoplanetary disks (Bouwman et al. 2001; van Boekel et al. 2003; Juhász et al. 2010; Miotello et al. 2012); however, they effectively trace the dust content only of the inner disk and its surface…”
C2D Spitzer-IRS spectra of disks around T Tauri stars. II. PAH emission features (2006, methodology): “Evidence for grain growth has been found from modeling of the silicate features from Herbig Ae/Be (hereafter HAeBe) (van Boekel et al. 2003) and T Tauri disks (Przygodda et al. 2003; KesslerSilacci et al. 2005, 2006) and more indirectly from the modeling of the observed H2 emission features from T…”
A 10 μm spectroscopic survey of Herbig Ae star disks: Grain growth and crystallization (2005, methodology): “By use of the LNIR/LIR ratio (van Boekel et al. 2003) we compare the near-IR SED to the mid-IR SED.”
ISO spectroscopy of disks around Herbig Ae/Be stars , (2004, background): “…silicate grains (∼0.1 µm) cause a distinct feature that peaks around 9.7 micron, while larger grains (∼2 µm) induce a broader, less pronounced feature with a peak towards longer wavelengths (Bouwman et al. 2001). van Boekel et al. (2003) interpret this sequence in terms of grain growth in the disk.”
The global gas and dust budget of the Large Magellanic Cloud: AGB stars and supernovae, and the impact on the ISM evolution (2009, methodology): “Hillier et al. (2001) suggested a gas mass-loss rate of 1 × 10−3 M yr−1 for η Car using a formula from Wright & Barlow (1975); near-infrared interferometric observations suggested 1.6 × 10−3 M yr−1 (van Boekel et al. 2003) for η Car.”
Keplerian discs around post-AGB stars: a common phenomenon? (2006, methodology): “Other examples exist and there is substantial observational evidence that the systems are all likely surrounded by a circumstellar orbiting disc (Van Winckel 2003).”
CRYSTALLINE SILICATES AND DUST PROCESSING IN THE PROTOPLANETARY DISKS OF THE TAURUS YOUNG CLUSTER (2007, methodology): “This alternative has been fruitful before in the analysis of Class II YSO spectra (e.g., Kessler-Silacci et al. 2005, 2006) and Herbig Ae/Be stars (e.g., Bouwman et al. 2001; van Boekel et al. 2003).”