Difference between revisions of "Triggers:YSOecl"
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Jump to navigationJump to searchAleks.scholz (talk | contribs) (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 | + | * 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 | + | * 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 | + | * YLW 16 A: has smaller eclipses- http://adsabs.harvard.edu/abs/2013A%26A...554A.110P |
Revision as of 14:41, 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:
- 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
- YLW 16 A: has smaller eclipses- http://adsabs.harvard.edu/abs/2013A%26A...554A.110P
