Survival time of preplanetary nebulae debris.

Details Survival time of preplanetary nebulae debris. Survival time of preplanetary nebulae debris.

Nov 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993rmxaa..27..121f&link_type=abstract

Revista Mexicana de Astronomia y Astrofisica, Vol. 27, p. 121 - 124

Astronomy and Astrophysics

Astronomy

Planetary Nebulae: Planetary Systems, Planetary Nebulae: Oh Masers

Scientific paper

In a previous paper (Fierro, 1993) the author suggested the possibility and the consequences of having planets, rings and ring arcs around planetary nebulae and the interactions they might have with the nebulae, concerning their morphology and chemical composition. In the present paper the author calculates the survival time of an ice planet around a newly formed preplanetary nebula and the conditions that would have to exist in order for its evaporation to account for the OH molecules that produce OH maser emission observed in some possible progenitors.

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