Astrophysics of Dust

By A. Witt, G. Clayton, B. Draine. 2004

238 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/d76b3f9c1cb7feefc46d26919981e08c3e3df9c7

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

1. E. Chiang
2. B. Draine
3. J. Jørgensen
4. A. Fraisse
5. D. Massa
6. F. Bresolin
7. S. Bisschop
8. E. V. van Dishoeck

Citations in the corpus

• An Analysis of the Shapes of Interstellar Extinction Curves. V. The IR-through-UV Curve Morphology (2007, methodology): “Subject headings: ISM:dust,extinction — methods:data analysis”
• Testing grain-surface chemistry in massive hot-core regions (2007, background): “…observations have shown that even on scales as small as a few thousand AU, there may be strong chemical differentiation, e.g., oxygen-bearing molecules peaking at a different position than nitrogen-bearing species (Liu 2005; Blake et al. 1996, 1987; Wyrowski et al. 1999; Sutton et al. 1995).”
• POLARIZED FAR-INFRARED AND SUBMILLIMETER EMISSION FROM INTERSTELLAR DUST (2008, background): “…wavelength dependence, with the polarization at 350 µm observed to be significantly smaller than the 100 µm and 850 µm polarization (Vaillancourt 2002; Hildebrand & Kirby 2004; Hildebrand 2005; Vaillancourt 2007), which has been interpreted as indicating two separate populations of emitting grains…”
• Particle Pileups and Planetesimal Formation (2003, background): “No boundary condition is required at the inner boundary, rin ¼ 0:5 AU, where material leaves the grid.”
• EXTRAGALACTIC CHEMICAL ABUNDANCES: DO H ii REGIONS AND YOUNG STARS TELL THE SAME STORY? THE CASE OF THE SPIRAL GALAXY NGC 300 (2009, background): “Quantifying the amount of oxygen that is locked up into dust grains is made difficult by the uncertainties in the total (gas-phase + dust) amount that is assumed, and usually taken from the composition of the Sun, B stars or young cool stars (Sofia 2004).”