LAMOST Reveals Long-lived Protoplanetary Disks

Fuente: arXiv
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Main Authors: Wang, Xiao-Long, Fang, Min, Liu, Yao, Zhang, Miao-Miao, Cui, Wen-Yuan
Format: Preprint
Published: 2025
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author Wang, Xiao-Long
Fang, Min
Liu, Yao
Zhang, Miao-Miao
Cui, Wen-Yuan
author_facet Wang, Xiao-Long
Fang, Min
Liu, Yao
Zhang, Miao-Miao
Cui, Wen-Yuan
contents While both observations and theories demonstrate that protoplanetary disks are not expected to live much longer than $\sim$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.
format Preprint
id arxiv_https___arxiv_org_abs_2501_04295
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle LAMOST Reveals Long-lived Protoplanetary Disks
Wang, Xiao-Long
Fang, Min
Liu, Yao
Zhang, Miao-Miao
Cui, Wen-Yuan
Astrophysics of Galaxies
While both observations and theories demonstrate that protoplanetary disks are not expected to live much longer than $\sim$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.
title LAMOST Reveals Long-lived Protoplanetary Disks
topic Astrophysics of Galaxies
url https://arxiv.org/abs/2501.04295