Why Are Two Stars Leaving Our Galaxy?

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Discussion Overview

The discussion centers around the phenomenon of two stars leaving the Milky Way galaxy, exploring the implications of their high velocities and the potential visual effects associated with such movement. The scope includes theoretical considerations and conceptual clarifications regarding stellar behavior and interactions.

Discussion Character

  • Exploratory
  • Technical explanation
  • Conceptual clarification

Main Points Raised

  • Some participants note that two exiled stars are leaving the galaxy at high speeds.
  • One participant questions whether hypervelocity stars leave a trail similar to a comet's dust tail.
  • Another participant argues that there is no reason for a star to leave a fiery tail, explaining that comet tails are produced by specific mechanisms related to solar radiation and winds.
  • This participant suggests that if a star were to interact closely with a powerful O/B star, it might produce a shadow in the stellar wind nebula rather than a tail.

Areas of Agreement / Disagreement

Participants express differing views on whether hypervelocity stars can leave a visible trail, indicating a lack of consensus on this aspect of stellar behavior.

Contextual Notes

The discussion includes assumptions about the conditions under which stars might interact and the definitions of terms like "tail" and "shadow" in the context of stellar winds.

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Does a hypervelocity star leave a fiery trail, like a comet's dust tail?
 
There is no reason for a star of any velocity to "leave a fiery tail".

A comet's tail is produced by the radiation pressure (dust tail) and solar wind/magnetic field (ion tail) coming from the Sun.

If a star is moving close by another very powerful O/B star then the radiation pressure and possible stellar wind emanating from that could act of the former's corona and produce some sort of tail, however ithe passing star is more likely to produce a shadow in the O/B stellar wind nebula, similar to the Cone nebula.

Garth
 

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