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![Schematic view for the formation of Bubble Nebula NGC 7635 [10]. Expanding wind hits the inner shock (dashed line), then kinetic energy is converted into thermal energy, which pushes a shell (thick line) into H II region (B), then pushes a shell (double line) into the interstellar medium (C).](publication/310897889/figure/fig2/AS:433009741570049@1480248975087/Schematic-view-for-the-formation-of-Bubble-Nebula-NGC-7635-10-Expanding-wind-hits-the.png)
Schematic view for the formation of Bubble Nebula NGC 7635 [10]. Expanding wind hits the inner shock (dashed line), then kinetic energy is converted into thermal energy, which pushes a shell (thick line) into H II region (B), then pushes a shell (double line) into the interstellar medium (C).
Source publication
Bubble Nebula is a bubble formed by the interaction between the stellar wind of BD+60°2522 with ambient interstellar gas. We use a web-based stellar evolution code, the EZ- web, to construct the evolution of BD+60°2522. From the evolution, we obtain the age of the system needed for the interstellar bubbles model. Then from the model, we determine p...
Context in source publication
Context 1
... is shown in figure 2, the interaction yields four regions: stellar wind region (a), inner shocked stellar wind region (b) with radius R1, outer shocked interstellar gas region (c) with radius R2, and ambient interstellar gas (d). [10] and [1] applied this model to the formation of Bubble Nebula NGC 7635, as is shown in figure 3. [10]. ...
