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Runaway Growth of Fractal Dust Grains
2015 (English)In: WHY GALAXIES CARE ABOUT AGB STARS III: A CLOSER LOOK IN SPACE AND TIME, ASTRONOMICAL SOC PACIFIC , 2015, Vol. 497, 393-394 p.Conference paper (Refereed)Text
Abstract [en]

Fractal grains have a large surface area, which leads to more efficient condensation. The special limiting case where the volume-area ratio is constant (corresponding to, e.g., a very rough grain surface or non-compact aggregates) is particularly interesting, as well as convenient, from a mathematical point of view. If dust grains from AGB stars have 'rough surfaces,' that may have important implications for our understanding of dust and wind formation in AGB stars.

Place, publisher, year, edition, pages
ASTRONOMICAL SOC PACIFIC , 2015. Vol. 497, 393-394 p.
National Category
Astronomy, Astrophysics and Cosmology
Identifiers
URN: urn:nbn:se:kth:diva-184943ISI: 000371098100075OAI: oai:DiVA.org:kth-184943DiVA: diva2:918319
Note

QC 20160411

Available from: 2016-04-11 Created: 2016-04-07 Last updated: 2016-04-11Bibliographically approved

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