Difference between revisions of "Triggers:YSOecl"

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(Created page with "== Eclipsing young stellar objects == Characteristics: * long-lasting eclipses by disk material * shapes can be irregular * timescales days to years * high amplitudes possible (...")
 
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Examples:
 
Examples:
  
* KH15D recurrent, but changing eclipses- see Herbst et al. 2012 http://adsabs.harvard.edu/abs/2010AJ....140.2025H
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* KH15D: recurrent, but changing eclipses- see Herbst et al. 2012 http://adsabs.harvard.edu/abs/2010AJ....140.2025H
* RW Aur singular event - http://figshare.com/articles/A_huge_eclipse_in_the_young_star_RW_Aur/92169
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* RW Aur: singular event - http://figshare.com/articles/A_huge_eclipse_in_the_young_star_RW_Aur/92169
* YLW 16 A has smaller eclipses- http://adsabs.harvard.edu/abs/2013A%26A...554A.110P
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* YLW 16 A: has smaller eclipses- http://adsabs.harvard.edu/abs/2013A%26A...554A.110P

Revision as of 15:41, 19 July 2013

Eclipsing young stellar objects

Characteristics:

  • long-lasting eclipses by disk material
  • shapes can be irregular
  • timescales days to years
  • high amplitudes possible (several mags)
  • very few known, every new detection would help

Examples: