Publication Abstracts

Gilman 1969

Gilman, R.C., 1969: On the composition of circumstellar grains. Astrophys. J., 155, L185-L187, doi:10.1086/180332.

On the basis of calculations of molecular equilibrium, it appears likely that circumstellar grains of oxygen-rich cool stars will be composed mainly of refractory silicates such as Mg2SiO4 and Al2SiO5. For carbon-rich stars the grains are mainly carbon, while for the transition stars silicon carbide predominates.

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BibTeX Citation

  author={Gilman, R. C.},
  title={On the composition of circumstellar grains},
  journal={Astrophysical Journal},

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RIS Citation

ID  - gi01100t
AU  - Gilman, R. C.
PY  - 1969
TI  - On the composition of circumstellar grains
JA  - Astrophys. J.
JO  - Astrophysical Journal
VL  - 155
SP  - L185
EP  - L187
DO  - 10.1086/180332
ER  -

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