New Low-mass Accretors in the Scorpius-Centaurus OB Association

Simon J. Murphy, Warrick A. Lawson, Joao Bento

    Research output: Contribution to journalArticlepeer-review

    Abstract

    We describe the serendipitous discovery of two new lithium-rich M5 members of the Scorpius-Centaurus OB Association (Sco-Cen). Both stars exhibit large 12 and 22 μm excesses and strong, variable Hα emission which we attribute to accretion from circumstellar discs. Such stars are thought to be incredibly rare at the ∼16 Myr median age of much of Sco-Cen. The serendipitous discovery of two accreting stars hosting large quantities of circumstellar material may be indicative of a sizeable age spread in Sco-Cen, or further evidence that disc dispersal and planet formation time-scales are longer around lower-mass stars.

    Original languageEnglish
    Pages (from-to)58-62
    Number of pages5
    JournalProceedings of the International Astronomical Union
    Volume10
    DOIs
    Publication statusPublished - 2015

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