Relation of SiO maser emission to IR radiation in evolved stars based on the MSX observation

Details Relation of SiO maser emission to IR radiation in evolved stars based on the MSX observation Relation of SiO maser emission to IR radiation in evolved stars based on the MSX observation

2002-01-06

arxiv.org/abs/astro-ph/0201073v1

Astronomy and Astrophysics

Astrophysics

11 pages, 4 figures, to appear in ApJL

Scientific paper

10.1086/339439

Based on the space MSX observation in bands A(8$\mu$m), C(12$\mu$m), D(15$\mu$m) and E(21$\mu$m), and the ground SiO maser observation of evolved stars by the Nobeyama 45-m telescope in the v=1 and v=2 J=1-0 transitions, the relation between SiO maser emission and mid-IR continuum radiation is analyzed. The relation between SiO maser emission and the IR radiation in the MSX bands A, C, D and E is all clearly correlated. The SiO maser emission can be explained by a radiative pumping mechanism according to its correlation with infrared radiation in the MSX band A.

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