Confirmation of a gapped primordial disk around LkCa 15
Catherine Espaillat, Nuria Calvet, Kevin L. Luhman, James Muzerolle,, and Paola D'Alessio

TL;DR
This study confirms the presence of an optically thick inner disk in LkCa 15, revealing a gapped primordial disk structure likely caused by forming planets, advancing understanding of disk evolution and planet formation.
Contribution
The paper provides direct spectroscopic evidence of an optically thick inner disk in LkCa 15, confirming the pre-transitional disk structure and supporting planet formation as the gap-clearing mechanism.
Findings
Confirmation of an optically thick inner disk in LkCa 15
Detection of a gapped disk structure
Implication of forming planets clearing the gap
Abstract
Recently, analysis of near-infrared broad-band photometry and Spitzer IRS spectra has led to the identification of a new "pre-transitional disk" class whose members have an inner optically thick disk separated from an outer optically thick disk by an optically thin gap. This is in contrast to the "transitional disks" which have inner disk holes (i.e. large reductions of small dust from the star out to an outer optically thick wall). In LkCa 15, one of these proposed pre-transitional disks, detailed modeling showed that although the near-infrared fluxes could be understood in terms of optically thick material at the dust sublimation radius, an alternative model of emission from optically thin dust over a wide range of radii could explain the observations as well. To unveil the true nature of LkCa 15's inner disk we obtained a medium-resolution near-infrared spectrum spanning the…
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Taxonomy
TopicsStellar, planetary, and galactic studies · Astrophysics and Star Formation Studies · Astronomy and Astrophysical Research
