Poster Open Access
Peter Pan Disks: Long-lived Accretion Disks Around ≥20 Myr Low-Mass Stars
Silverberg, Steven M.;
Kuchner, Marc J.
Editor(s)
Wolk, ScottThis poster summarizes Silverberg et al. (2020) and subsequent new results in the literature regarding “Peter Pan” disks, a class of substantial M star disks with spectroscopic evidence of accretion in young stellar associations (YSAs) at ages ≥20 Myr—i.e. they seem to "never grow up." We outline the ensemble characteristics of the eight known Peter Pan disks from optical and near-IR spectroscopy, ALMA observations of WISEA J080822.18-644357.3 (J0808; the prototypical Peter Pan disk), and optical light curves, including TESS Cycle 3 observations of J0808. We find that these objects most plausibly represent long-lived CO-poor primordial disks, or "hybrid" disks, exhibiting both debris and primordial-disk features. We finally outline Disk Detective v2.0, a citizen science project for identifying circumstellar disks in WISE data that is explicitly designed to leverage Gaia to search for new Peter Pan disks.
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silverberg_coolstars_20half_PeterPanDisks_finalv3.pdf
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| All versions | This version | |
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| Data volume | 40.2 MB | 40.2 MB |
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- Publication date:
- February 27, 2021
- DOI:
-
- Keyword(s):
- Young stars Circumstellar disks Accretion disks Variability
- Meeting:
- The 20.5th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun (CS20.5), virtually anywhere, March 2-4, 2021
- Communities:
- License (for files):
- Creative Commons Attribution 4.0 International