The role of water chemistry in accretion disks of FU Ori-stars

Details The role of water chemistry in accretion disks of FU Ori-stars The role of water chemistry in accretion disks of FU Ori-stars

May 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992aas...180.4312d&link_type=abstract

American Astronomical Society, 180th AAS Meeting, #43.12; Bulletin of the American Astronomical Society, Vol. 24, p.798

Astronomy and Astrophysics

Astronomy

Scientific paper

Under certain circumstances that are mainly determined by the opacity, accretion disks in stellar systems may turn unstable. We discuss the influence of the water molecule on the stability of accretion disks in FU Ori-type stars. Furthermore, we present results of numerical models that indicate that the emerging instability is capable of changing its own environment in a non-reversible way such that the short- and long-term evolution of FU Ori-accretion disks may be governed by this instability and its self-regulatory capability.

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