arXiv Analytics

Sign in

arXiv:1301.2867 [astro-ph.SR]AbstractReferencesReviewsResources

Crystalline Silicates in Evolved Stars. I. Spitzer/IRS Spectroscopy of IRAS16456-3542, 18354-0638, and 23239+5754

B. W. Jiang, Ke Zhang, Aigen Li, C. M. Lisse

Published 2013-01-14Version 1

We report the Spitzer Infrared Spectrograph (IRS) observations of three evolved stars: IRAS 16456-3542, 18354-0638, and 23239+5754. The 9.9--37.2um Spitzer/IRS high resolution spectra of these three sources exhibit rich sets of enstatite-dominated crystalline silicate emission features. IRAS 16456-3542 is extremely rich in crystalline silicates, with >90% of its silicate mass in crystalline form, the highest to date ever reported for crystalline silicate sources.

Related articles: Most relevant | Search more
arXiv:1101.3757 [astro-ph.SR] (Published 2011-01-19)
Lithium abundances and extra mixing processes in evolved stars of M67
arXiv:2307.10452 [astro-ph.SR] (Published 2023-07-19)
Mass Loss in Evolved Stars
arXiv:1904.05425 [astro-ph.SR] (Published 2019-04-10)
Photodissociation of CO in the outflow of evolved stars