SiO masers in late-type giant stars - Jovian planets engulfed

Details SiO masers in late-type giant stars - Jovian planets engulfed SiO masers in late-type giant stars - Jovian planets engulfed

Jul 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apj...330..986s&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 330, July 15, 1988, p. 986-991.

Astronomy and Astrophysics

Astrophysics

19

Giant Stars, Late Stars, Masers, Planetary Systems, Variable Stars, Mira Variables, Silicon Oxides, Stellar Atmospheres, Vaporizing, Very Long Base Interferometry

Scientific paper

The hypothesis is explored that SiO masers in late-type giant stars may be associated with the magnetospheres and orbital wakes of Jovian planets, with the vaporization of rocky satellites adding SiO molecules. What would happen to the solar system if the sun became a Mira variable is examined. The hypothetical results are compared with available observations, and predictions are made regarding observable, long-time variations in the positions and velocities of maser sources.

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