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    1. Introduction
    ... Bright-rimmed clouds are surrounded and compressed by a curved ionization/shock front on at least one side of their surface. ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/15_1/ogura/paper/node1.html -- 51.7 Кб -- 08.04.2016
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    2. Background
    ... For the latter class, the emission might be part of an expanding-shell shock front, or an ionization front on a relatively stationary Hб  I structure. ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/15_1/mcintyre/paper/node1.html -- 52.9 Кб -- 08.04.2016
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    3. No Title
    ... These models show the importance of ionization fronts for the structure of planetary ... the outer shell is formed by the ionization front while the inner shell is swept-up ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/people/plintel/groups/lsse/agb/940601/940601.html -- 67.8 Кб -- 12.04.2016
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    4. The Orion Nebula
    ... Behind the HII region is an ionization front and photodissociation region which is the interface between the HII region and the molecular cloud; this has a thickness of about 10 -4 б pc (O'Dell 1993). ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/18_1/schultz/paper/node3.html -- 51.7 Кб -- 08.04.2016
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    5. No Title
    ... Furthermore the passing through of the ionization front may modify the density distribution in the slow wind, leading to the ... I consider how the different phases of ionization fronts and wind swept bubbles can be observationally distinguished. ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/people/plintel/groups/lsse/agb/950801/950801.html -- 75.8 Кб -- 12.04.2016
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    6. http://www.atnf.csiro.au/people/Ray.Norris/papers/n204.pdf
    ... in the head are, however, reduced and therefore the ionization front is not completely stalled but advances into the densest ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/people/Ray.Norris/papers/n204.pdf -- 1716.8 Кб -- 07.10.2010
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    7. Discussion
    ... We also see regions in SN remnants where there are a series of ionization fronts, some green while others are yellow and red illustrating the complex ionization structure and interaction between collisions and radiation. ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/17_2/bessell/paper/node3.html -- 61.4 Кб -- 08.04.2016
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    8. Basic mechanisms of thermal emission
    ... in regions with high densities (where collisions are relatively more important) and near dynamical features such as contact discontinuities, ionization fronts and shock waves (where density gradients and time-dependent processes might be important ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/15_1/cram/paper/node2.html -- 59.2 Кб -- 08.04.2016
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    9. http://www.atnf.csiro.au/research/masermeeting/web_papers/301_Fish.pdf
    ... 2003) Wa t e r Water masers associated with low-mass protostars preferentially close to ionization front, suggesting triggered star formation truncated after ~105 years (Healy et al. ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/research/masermeeting/web_papers/301_Fish.pdf -- 2200.2 Кб -- 25.03.2007
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    10. No Title
    ... While, model 2 has a thicker shell that drops off as r resulting in the ionization front stopping in the thick shell and a high density ionized region immediately surrounded by a neutral shell. ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/people/plintel/groups/lsse/agb/951201/951201.html -- 80.6 Кб -- 12.04.2016
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