Dust in brown dwarfs. V. Growth and evaporation of dirty dust grains

2006

143 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Mechanics of Materials

View Paper: https://www.semanticscholar.org/paper/4843b18bf90b376bbb482f602a5ae55e0df4ff18

Citations in the corpus

• NEGLECTED CLOUDS IN T AND Y DWARF ATMOSPHERES (2012, unknown): “2011, ApJ, 743, 50 de Kok, R. J., Helling, C., Stam, D. M., Woitke, P., & Witte, S.2011, A&A, 531, A67 Dupuy, T. J., & Liu, M. C. 2012, ApJS, 201, 19 Faherty, J. K., et al. 2012, ApJ, 752, 56 Fegley, B. J., & Lodders, K. 1994, Icarus, 110, 117 —.”
• The Transit Light Source Effect: False Spectral Features and Incorrect Densities for M-dwarf Transiting Planets (2017, unknown): “…& Baron 1999), with the DRIFT-PHOENIX model grids including additional physics describing the formation and condensation of mineral dust clouds (Woitke & Helling 2003, 2004; Helling & Woitke 2006; Helling et al. 2008a,b; Witte et al. 2009) that is applicable to late M dwarfs and brown dwarfs.”
• On the Cool Side: Modeling the Atmospheres of Brown Dwarfs and Giant Planets (2014, unknown): “A unique cloud modeling paradigm has been developed by Helling et al. in a series of papers (e.g., Helling et al. 2001; Helling & Woitke 2006; Helling et al. 2008a,b, and references therein).”
• Too little radiation pressure on dust in the winds of oxygen-rich AGB stars (2006, unknown): “For each condensate we take the maximum possible dust volume per massL3,max given by element conservation constraints, e. g.LMg2SiO43,max = Min { 1 2ǫMg, ǫSi, 1 4ǫO } VMg2SiO4 n〈H〉/ρ wheren〈H〉 is the hydrogen nuclei density,ǫk the abundance of elementk andVMg2SiO4 the monomer volume of Mg2SiO4 (see ”
• A comparison of chemistry and dust cloud formation in ultracool dwarf model atmospheres (2008, unknown): “Nucleation, growth/evaporation and gravitational settling are source terms of these equations (Woitke & Helling 2003; Helling & Woitke 2006).”
• QUANTITATIVELY ASSESSING THE ROLE OF CLOUDS IN THE TRANSMISSION SPECTRUM OF GJ 1214b (2013, unknown): “S. K. Ateya, J. B. Pollack, & M. S.Matthews (Tucson: Univ. of Arizona Press), 487–512 Gibbard, S. G., de Pater, I., Roe, H. G., Martin, S., Macintosh, B. A., & Max, C. E. 2003, Icarus, 166, 359 Hammel, H. B., et al. 1989, Science, 245, 1367 Hauschildt, P. H., Allard, F., Ferguson, J., Baron, E., & A”
• Detection of atmospheric haze on an extrasolar planet: the 0.55–1.05 μm transmission spectrum of HD 189733b with the Hubble Space Telescope (2007, unknown): “Strong signatures of clouds and hazes are observed in the spectra of brown dwarfs with similar atmospheric temperatures (Helling & Woitke 2006).”
• A Unified Theory for the Atmospheres of the Hot and Very Hot Jupiters: Two Classes of Irradiated Atmospheres (2007, unknown): “We think that opacity due to TiO/VO is a natural explanation, but more work needs to be done to understand the abundances of these molecules at low pressure in these dynamic atmospheres, such as a non-equilibrium cloud condensation model (see Helling & Woitke 2006, and §7.1).”