Processing of silicate dust grains in Herbig Ae/Be systems

By J. Bouwman, G. Meeus, A. D. Koter, S. Hony, C. Dominik, L. Waters. 2001

266 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/ce471472de2ba42d38f8fca2ca2d5b21d611c941

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In Astronomy and Astrophysics

Citations in the corpus

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.”
Spitzer IRS Spectroscopy of IRAS-discovered Debris Disks (2006, result): “The crystalline silicate fraction for HR 7012 appears extremely high; however, those of the other debris disks are consistent with measurements toward pre-main sequence T-Tauri and Herbig AeBe stars (Sargent et al. 2006; Bouwman et al. 2001).”
A reconsideration of disk properties in Herbig Ae stars (2001, background): “Variations in the grain size and in the proportion of the various materials from star to star are seen in the ISO spectra of HAe stars (Bouwman et al. 2001).”
Grain growth in the inner regions of Herbig Ae/Be star disks (2003, result): “Similar changes in dust composition have been found in the passive disks surrounding, in particular, Herbig Ae/Be (HAEBE) stars (e.g. Malfait et al. 1998; Bouwman et al. 2001, hereafter BO01; Meeus et al. 2001, hereafter ME01).”
ISO spectroscopy of disks around Herbig Ae/Be stars , (2004, background): “The spectral signature at 11.3 micron, as well as many features at longer wavelengths which are not included in the analysis presented in this paper, is linked to crystalline silicates (Malfait et al. 1998, 1999; van den Ancker et al. 2000a,b; Bouwman et al. 2000, 2001).”
The Absence of Crystalline Silicates in the Diffuse Interstellar Medium (2004, background): “They are detected in debris disk object Pic (Knacke et al. 1993), in some T Tauri stars (Honda et al. 2003), and are quite common in the more massive Herbig Ae/Be stars (e.g., Bouwman et al. 2001; Meeus et al. 2001).”
Probing dust grain evolution in IM Lupi's circumstellar disc. Multi-wavelength observations and mo (2008, background): “…study of the 10µm feature provides quantitative information on the composition and size of the grains responsible for the observed emission (e.g. Bouwman et al. 2001, van Boekel et al. 2005, Apai et al. 2005, Schegerer et al. 2006 or more recently Meŕın et al. 2007, Bouy et al. 2008 and…”
Triggered massive-star formation on the borders of Galactic H II regions I. A search for "collect and collapse" candidates (2004, unknown): “Most present a continuum emission increasing with wavelength; some exhibit a strong silicate emission near 10 µm, others PAH emission bands (Bouwman et al. 2001; Meeus et al. 2001).”
c2d Spitzer IRS Spectra of Disks around T Tauri Stars. I. Silicate Emission and Grain Growth (2005, background): “Studies of 10 m silicate emission fromHerbig Ae-Be stars (HAEBEs) and T Tauri stars (TTs) with disks show early evidence of the growth of these surface-layer grains from 0.1 to 2.0 m (see, e.g., Bouwman et al. 2001; van Boekel et al. 2003).”
Dust grain growth in ρ-Ophiuchi protoplanetary disks (2010, methodology): “8, are interpreted in terms of grain growth to micron sizes (Bouwman et al. 2001; Kessler-Silacci et al. 2006).”
The origin of crystalline silicates in the Herbig Be star HD 100546 and in comet Hale-Bopp (2003, background): “In a series of papers, we have studied the dust emission from HAEBE stars (Waelkens et al. 1996; Malfait et al. 1998; Malfait et al. 1999, van den Ancker et al. 2000, 2001; Bouwman et al. 2000, 2001; Meeus et al. 2001), focusing on the mineralogical composition of the dust.”
A 10 μm spectroscopic survey of Herbig Ae star disks: Grain growth and crystallization (2005, background): “The ISO spectra reveal a mineralogy dominated by the crystalline silicates forsterite and enstatite, i.e. Mg-rich, Fe-poor materials (e.g. Malfait et al. 1998b; Bouwman et al. 2001; Meeus et al. 2001, hereafter ME01).”
INTERSTELLAR DUST GRAINS (2003, background): “Bouwman et al. (2001) find that 5-10% of the olivine mass is crystalline in the dust around Herbig Ae/Be stars.”
Turbulent Radial Mixing in the Solar Nebula as the Source of Crystalline Silicates in Comets (2000, background): “Crystalline silicates have been detected in disks around pre-main-sequence Herbig Ae/Be stars (e.g., Malfait et al. 1998; Bouwman et al. 2001).”
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…”
ISO Spectroscopy of Gas and Dust: From Molecular Clouds to Protoplanetary Disks (2004, background): “Bouwman et al. (2001) argue on the basis of correlations between features that grain growth from sub-micron to micron-sized grains dominates the shift.”
Dust properties of protoplanetary disks in the Taurus-Auriga star forming region from millimeter wavelengths (2009, background): “The boxy features with low feature-tocontinuum ratios are interpreted as grain growth to micron size (Bouwman et al. 2001).”