Disc clearing of young stellar objects: evidence for fast inside-out dispersal

Author(s)
C. M. Koepferl, B. Ercolano, J. Dale, P. S. Teixeira, T. Ratzka, L. Spezzi
Abstract

The time-scale over which and the modality by which young stellar

objects (YSOs) disperse their circumstellar discs dramatically influence

the eventual formation and evolution of planetary systems. By means of

extensive radiative transfer modelling, we have developed a new set of

diagnostic diagrams in the infrared colour-colour plane (K - [24] versus

K - [8]), to aid with the classification of the evolutionary stage of

YSOs from photometric observations. Our diagrams allow the

differentiation of sources with unevolved (primordial) discs from those

evolving according to different clearing scenarios (e.g. homologous

depletion versus inside-out dispersal), as well as from sources that

have already lost their disc. Classification of over 1500 sources in 15

nearby star-forming regions reveals that approximately 39 per cent of

the sources lie in the primordial disc region, whereas between 31 and 32

per cent disperse from the inside-out and up to 22 per cent of the

sources have already lost their disc. Less than 2 per cent of the

objects in our sample lie in the homogeneous draining regime.

Time-scales for the transition phase are estimated to be typically a few

105 yr independent of stellar mass. Therefore, regardless of

spectral type, we conclude that currently available infrared photometric

surveys point to fast (of the order of 10 per cent of the global disc

lifetime) inside-out clearing as the preferred mode of disc dispersal.

Organisation(s)
Department of Astrophysics
External organisation(s)
Ludwig-Maximilians-Universität München, Excellence Cluster Universe, European Southern Observatory (Germany)
Journal
Monthly Notices of the Royal Astronomical Society
Volume
428
Pages
3327-3354
No. of pages
28
ISSN
0035-8711
DOI
https://doi.org/10.1093/mnras/sts276
Publication date
02-2013
Peer reviewed
Yes
Austrian Fields of Science 2012
103004 Astrophysics, 103003 Astronomy
Keywords
Portal url
https://ucrisportal.univie.ac.at/en/publications/14d62154-3844-4607-b8c4-55cca2169b3b