Are the silicate crystallinities of oxygen-rich evolved stars related to their mass loss rates?
2018 ◽
Vol 14
(S343)
◽
pp. 425-426
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AbstractA sample of 28 oxygen-rich evolved stars is selected based on the presence of crystalline silicate emission features in their ISO/SWS spectra. The crystallinity, measured as the flux fraction of crystalline silicate features, is found not to be related to mass loss rate that is derived from fitting the spectral energy distribution.
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2018 ◽
Vol 14
(S343)
◽
pp. 464-465
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1999 ◽
Vol 191
◽
pp. 379-388
1999 ◽
Vol 192
◽
pp. 95-99
2020 ◽
Vol 492
(4)
◽
pp. 5994-6006
◽
Keyword(s):
2018 ◽
Vol 14
(S343)
◽
pp. 458-459
Keyword(s):
2015 ◽
Vol 11
(A29B)
◽
pp. 454-454
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