Molecular line emission from gravitationally unstable protoplanetary disks

Desika Narayanan, Craig A. Kulesa, Alan Boss, Christopher K Walker

Research output: Contribution to journalArticle

24 Citations (Scopus)

Abstract

In the era of high-resolution submillimeter interferometers, it will soon be possible to observe the neutral circum-stellar medium directly involved in gas giant planet (GGP) formation at physical scales previously unattainable. In order to explore possible signatures of GGP formation via disk instabilities, we have combined a three-dimensional (3D), nonlocal thermodynamic equilibrium (LTE) radiative transfer code with a 3D, finite differences hydrodynamical code to model molecular emission lines from the vicinity of a 1.4MJ self-gravitating proto-GGP. Here we explore the properties of rotational transitions of the commonly observed dense gas tracer, HCO+ . Our main results are as follows: (1) Very high lying HCO+ transitions (e.g., HCO+ J = 7-6) can trace dense clumps around circumstellar disks. Depending on the molecular abundance, the proto-GGP may be directly imageable by the Atacama Large Millimeter Array (ALMA). (2) HCO+ emission lines are heavily self-absorbed through the proto-GGP's dense molecular core. This signature is nearly ubiquitous and only weakly dependent on assumed HCO+ abundances. The self-absorption features are most pronounced at higher angular resolutions. Dense clumps that are not self-gravitating only show minor self-absorption features. (3) Line temperatures are highest through the proto-GGP at all assumed abundances and inclination angles. Conversely, due to self-absorption in the line, the velocity-integrated intensity may not be. High angular resolution interferometers such as the Submillimeter Array (SMA) and ALMA may be able to differentiate between competing theories of GGP formation.

Original languageEnglish (US)
Pages (from-to)1426-1436
Number of pages11
JournalAstrophysical Journal
Volume647
Issue number2 I
DOIs
StatePublished - Aug 20 2006

Fingerprint

gas giant planets
protoplanetary disks
planet
self absorption
gas
clumps
angular resolution
interferometer
high resolution
interferometers
signatures
local thermodynamic equilibrium
thermodynamic equilibrium
radiative transfer
inclination
tracers
thermodynamics
tracer
gases

Keywords

  • Circumstellar matter
  • Line: formation
  • Line: profiles
  • Planetary systems: formation
  • Planetary systems: protoplanetary disks
  • Radiative transfer

ASJC Scopus subject areas

  • Space and Planetary Science

Cite this

Molecular line emission from gravitationally unstable protoplanetary disks. / Narayanan, Desika; Kulesa, Craig A.; Boss, Alan; Walker, Christopher K.

In: Astrophysical Journal, Vol. 647, No. 2 I, 20.08.2006, p. 1426-1436.

Research output: Contribution to journalArticle

Narayanan, Desika ; Kulesa, Craig A. ; Boss, Alan ; Walker, Christopher K. / Molecular line emission from gravitationally unstable protoplanetary disks. In: Astrophysical Journal. 2006 ; Vol. 647, No. 2 I. pp. 1426-1436.
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