Exoplanetology: Exoplanets & Exomoons

LAMOST Reveals Long-lived Protoplanetary Disks

By Keith Cowing
Status Report
astro-ph.GA
January 9, 2025
Filed under , , , , , , ,
LAMOST Reveals Long-lived Protoplanetary Disks
Left: E(KS −W3) vs. E(KS −W4) color excess plot for our targets. Full disks, transitional disks, evolved disks and debris disks are shown as red circles, orange squares, cyan triangles and blue diamonds, respectively. The newly discovered Peter Pan disks are highlighted with additional blue pluses. The solid lines display the boundaries used to classify our targets into different categories (Esplin et al. 2014, 2018). Right: similar as the left panel, but shows the E(KS − W2) vs. E(KS − W3) color excess plot. — astro-ph.GA

While both observations and theories demonstrate that protoplanetary disks are not expected to live much longer than ∼10 Myr, several examples of prolonged disks have been observed in the past.

In this work, we perform a systematic search for aged YSOs still surrounded by protoplanetary disks in the M star catalog from the LAMOST archive.

We identify 14 sources older than 10 Myr, still surrounded by protoplanetary disks and with ongoing accretion activities, significantly improving the census of the category known as the Peter Pan disks.

The stellar parameters, variability and accretion properties of these objects, as well as their spatial distribution, are investigated. Nearly all of these objects are distributed far away from nearby associations and star forming regions, but show evidence of being members of open clusters.

Investigating the correlation between mass accretion rates and stellar masses, we find these long-lived disks accrete at systematically lower levels, compared to their younger counterparts with similar stellar masses. Studying the evolution of mass accretion rates with stellar ages, we find these aged disks follow similar trend as young ones.

Xiao-Long Wang, Min Fang, Yao Liu, Miao-Miao Zhang, Wen-Yuan Cui

Comments: 24 pages, 12 figures, 2 tables, Accepted for publication in AJ
Subjects: Astrophysics of Galaxies (astro-ph.GA)
Cite as: arXiv:2501.04295 [astro-ph.GA] (or arXiv:2501.04295v1 [astro-ph.GA] for this version)
https://doi.org/10.48550/arXiv.2501.04295
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Submission history
From: Xiao-Long Wang
[v1] Wed, 8 Jan 2025 05:42:32 UTC (1,726 KB)
https://arxiv.org/abs/2501.04295
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