Phenomenological Theory of the Photoevaporation Front Instability

Details Phenomenological Theory of the Photoevaporation Front Instability Phenomenological Theory of the Photoevaporation Front Instability

Jan 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ap%26ss.307..173r&link_type=abstract

Astrophysics and Space Science, Volume 307, Issue 1-3, pp. 173-177

Astronomy and Astrophysics

Astrophysics

1

Hii Regions, Ablation Front Instability, Eagle Nebula, Laboratory Astrophysics

Scientific paper

The dynamics of photoevaporated molecular clouds is determined by the ablative pressure acting on the ionization front. An important step in the understanding of the ensuing motion is to develop the linear stability theory for an initially flat front. Despite the simplifications introduced by linearization, the problem remains quite complex and still draws a lot of attention. The complexity is related to the large number of effects that have to be included in the analysis: acceleration of the front, possible temporal variation of the intensity of the ionizing radiation, the tilt of the radiation flux with respect to the normal to the surface, and partial absorption of the incident radiation in the ablated material. In this paper, we describe a model where all these effects can be taken into account simultaneously, and a relatively simple and universal dispersion relation can be obtained. The proposed phenomenological model may prove to be a helpful tool in assessing the feasibility of the laboratory experiments directed towards scaled modeling of astrophysical phenomena.

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