PREPRINT
3202103D-F537-495C-87ED-4935B939C7B7

Disentangling protoplanetary disk gas mass and carbon depletion through combined atomic and molecular tracers

J. A. Sturm, A. S. Booth, M. K. McClure, M. Leemker, E. F. van Dishoeck

Submitted on 19 September 2022

Abstract

The total disk gas mass and elemental C, N, O composition of protoplanetary disks are crucial ingredients for our understanding of planet formation. Measuring the gas mass is complicated, since H2 cannot be detected in the cold bulk of the disk and the elemental abundances with respect to hydrogen are degenerate with gas mass in all disk models. We present new NOEMA observations of CO, 13CO, C18O and optically thin C17O J=2-1 lines, and use additional high angular resolution Atacama Large Millimeter Array millimeter continuum and CO data to construct a representative model of LkCa 15. The transitions that constrain the gas mass and carbon abundance most are C17O 2-1, N2H+ 3-2 and HD 1-0. Using these three molecules we find that the gas mass in the LkCa 15 disk is Mg=0.010.004+0.01M, a factor of six lower than estimated before. The carbon abundance is C/H = (3±1.5)×105, implying a moderate depletion of elemental carbon by a factor of 3-9. All other analyzed transitions also agree with these numbers, within a modeling uncertainty of a factor of two. Using the resolved \ce{C2H} image we find a C/O ratio of 1, which is consistent with literature values of H2O depletion in this disk. The lack of severe carbon depletion in the LkCa 15 disk is consistent with the young age of the disk, but contrasts with the higher depletions seen in older cold transition disks. Combining optically thin CO isotopologue lines with N2H+ is promising to break the degeneracy between gas mass and CO abundance. The moderate level of depletion for this source with a cold, but young disk, suggests that long carbon transformation timescales contribute to the evolutionary trend seen in the level of carbon depletion among disk populations, rather than evolving temperature effects and presence of dust traps alone.

Preprint

Comment: 16 pages, 8 figures. Accepted for publication in A&A

Subjects: Astrophysics - Earth and Planetary Astrophysics; Astrophysics - Astrophysics of Galaxies

URL: https://arxiv.org/abs/2209.09286