Nikole Nielsen.pdf
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Nikole Nielsen.pdf
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arXiv:1211.1008, arXiv:1211.1380Amount of MgII vs Impact Parameter• Anti‐correlation between W r (2796) and D – 7.9 σ• Highest mass galaxies have larger EW at a given D• Mass segregation vanishes when normalizing by virialradius – 9.2 σ anti‐correlation• Amount and extent of MgII gas depends strongly on mass
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