Erratum: The shape and composition of interstellar silicate grains

By M. Min, L. Waters, A. D. Koter, J. Hovenier, L. Keller, F. Markwick-Kemper. 2008

144 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/a85367c884b9e970046096dc39b362546a65ac5a

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In Astronomy and Astrophysics

1. E. A. Petersen
2. G. Sloan
3. Igor Soszynski
4. M. Groenewegen
5. N. Mauron
6. E. Josselin

Citations in the corpus

• Luminosities and mass-loss rates of SMC and LMC AGB stars and red supergiants (2009, methodology): “Min et al. (2005, 2007) show that a DHS with fmax= 0.7 provides a good fit to the shape of the interstellar silicate feature at 10µm, while with a value of 0.4 they can reproduce the polarisation properties of quartz measured in laboratory data.”