Silicate Dust Emission in SR Variables

Details Silicate Dust Emission in SR Variables Silicate Dust Emission in SR Variables

Feb 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.224..419a&link_type=abstract

Astrophysics and Space Science, Volume 224, Issue 1-2, pp. 419-420

Astronomy and Astrophysics

Astrophysics

3

Stars: Agb, Stars: Variable, Stars: Mass-Loss

Scientific paper

We have investigated the IRAS LRS spectra of a sample of 56 Semiregular
(SR) variables with silicate dust features (class 2 n) and existing near
infrared photometry. We compare our results to similar work that has
been done on Mira variables by Little-Marenin & Little (1990).

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