Hydrogen sulfide detected in the protoplanetary disk of GG Tauri A
An international team of researchers has detected hydrogen sulfide emission from the dense protoplanetary disk around the star GG Tauri A. It is the first detection of this chemical compound in a protoplanetary disk. The finding is reported in a paper published August 2 on the arXiv pre-print server.
Located some 490 light-years away from the Earth in the Taurus-Auriga star-forming region, GG Tauri (GG Tau for short) is a quintuple system with the GG Tauri A (GG Tau A) triple star. GG Tau is known to have a dense ring located between 180 and 260 AU from it, and a large disk extending out to 800 AU. Due to its large size, low temperature (about 20 K) and large mass (about 0.15 solar masses), the disk is perceived by astronomers as an excellent target to search for cold molecular chemistry.
Recently, a group of astronomers led by Nguyen Thi Phuong of the University of Bordeaux in France, has conducted a chemical study of the circumstellar disk surrounding GG Tau A. Their research was focused on sulfur-bearing molecules, therefore, the scientists searched for hydrogen sulfide (H2S), carbon monosulfide (CS), sulfur monoxide (SO), and sulfur dioxide (SO2).
The study, carried out with the use of the NOrthem Extended Millimeter Array (NOEMA) interferometer located in Plateau de Bure in the French Alps, allowed the researchers to detect the hydrogen sulfide emission. As noted in the paper, this marks the first detection of that compound in a protoplanetary disk.
"Using NOEMA, we have observed the GG Tau A outer disk in several molecules. We report the first detection of H2S in a protoplanetary disk," the astronomers wrote in the paper.
According to the study, hydrogen sulfide is clearly detected with a peak signal-to-noise ratio of four in several channels. The scientists revealed that most of the line emission originates from the dense ring between 180 to 260 AU and extends up to 500 AU. They also found that the measured hydrogen sulfide column density is a factor of three greater than the upper limits for systems with disks like DM Tau, LkCa 15, MWC 480, and GO Tau, probably reflecting the larger disk mass of GG Tau A.
"Comparisons with other disks indicate that the detection of H2S appears to be facilitated by the large disk mass, but that the relative abundance ratios remain similar," the paper reads.
This, according to the researchers, indicates that GG Tau A could be a good test bed for studying chemistry in disks.
Besides hydrogen sulfide, the team also detected HCO+, H13CO+, and DCO+ in GG Tau A's protoplanetary disk. They added that the observed ratio of DCO+ to HCO+ is similar to those in other disks.
However, the researchers noted that they were not able to reproduce the observed column densities of sulfur-bearing molecules, even with low sulfur abundance, which suggests that the understanding of sulfur chemistry on dust grains is still incomplete.
More information: First detection of H2S in a protoplanetary disk. The dense GG Tau A ring, arXiv:1808.00652 [astro-ph.SR] arxiv.org/abs/1808.00652
Studying molecular species in protoplanetary disks is very useful to characterize the properties of these objects, which are the site of planet formation. We attempt to constrain the chemistry of S-bearing molecules in the cold parts of circumstellar disk of GG Tau A. We searched for H2S, CS, SO, and SO2 in the dense disk around GG Tau A with the NOrthem Extended Millimeter Array (NOEMA) interferometer. We detected H2S emission from the dense and cold ring orbiting around GG Tau A. This is the first detection of H2S in a protoplanetary disk. We also detected HCO+, H13CO+, and DCO+ in the disk. Upper limits for other molecules, CCS, SO2, SO, HC3N, and c-C3H2 are also obtained. The observed DCO+/HCO+ ratio is similar to those in other disks. The observed column densities, derived using our radiative transfer code DiskFit, are then compared with those from our chemical code Nautilus. The column densities are in reasonable agreement for DCO+, CS, CCS, and SO2. For H2S and SO, our predicted vertical integrated column densities are more than a factor of 10 higher than the measured values. Our results reinforce the hypothesis that only a strong sulfur depletion may explain the low observed H2S column density in the disk. The H2S detection in GG Tau A is most likely linked to the much larger mass of this disk compared to that in other T Tauri systems.
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