2017A&A...606A.125S


C.D.S. - SIMBAD4 rel 1.7 - 2020.07.10CEST02:19:25

2017A&A...606A.125S - Astronomy and Astrophysics, volume 606A, 125-125 (2017/10-1)

DCO+, DCN, and N2D+ reveal three different deuteration regimes in the disk around the Herbig Ae star HD 163296.

SALINAS V.N., HOGERHEIJDE M.R., MATHEWS G.S., OBERG K.I., QI C., WILLIAMS J.P. and WILNER D.J.

Abstract (from CDS):

Context. Deuterium fractionation has been used to study the thermal history of prestellar environments. Their formation pathways trace different regions of the disk and may shed light into the physical structure of the disk, including locations of important features for planetary formation.
Aims. We aim to constrain the radial extent of the main deuterated species; we are particularly interested in spatially characterizing the high and low temperature pathways for enhancing deuteration of these species.
Methods. We observed the disk surrounding the Herbig Ae star HD 163296 using ALMA in Band 6 and obtained resolved spectral imaging data of DCO+ (J=3-2), DCN (J=3-2) and N2D+ (J=3-2) with synthesized beam sizes of 0.53x0.42, 0.53x0.42, and 0.50x0.39, respectively. We adopted a physical model of the disk from the literature and use the 3D radiative transfer code LIME to estimate an excitation temperature profile for our detected lines. We modeled the radial emission profiles of DCO+, DCN, and N2D+, assuming their emission is optically thin, using a parametric model of their abundances and our excitation temperature estimates.
Results. DCO+ can be described by a three-region model with constant-abundance rings centered at 70AU, 150AU, and 260AU. The DCN radial profile peaks at about 60AU and N2D+ is seen in a ring at 160AU. Simple models of both molecules using constant abundances reproduce the data. Assuming reasonable average excitation temperatures for the whole disk, their disk-averaged column densities (and deuterium fractionation ratios) are 1.6-2.6x1012cm–2 (0.04-0.07), 2.9-5.2x1012cm–2 (∼0.02), and 1.6-2.5x1011cm–2 (0.34-0.45) for DCO+, DCN, and N2D+, respectively.
Conclusions. Our simple best-fit models show a correlation between the radial location of the first two rings in DCO+ and the DCN and N2D+ abundance distributions that can be interpreted as the high and low temperature deuteration pathways regimes. The origin of the third DCO+ ring at 260 AU is unknown but may be due to a local decrease of ultraviolet opacity allowing the photodesorption of CO or due to thermal desorption of CO as a consequence of radial drift and settlement of dust grains. The derived Df values agree with previous estimates of 0.05 for DCO+/HCO+ and 0.02 for DCN/HCN in HD 163296, and 0.3-0.5 for N2D+/N2H+ in AS 209, a T Tauri disk. The high N2D+/N2H+ confirms N2D+ as a good candidate for tracing ionization in the cold outer disk.

Abstract Copyright: © ESO, 2017

Journal keyword(s): astrochemistry - protoplanetary disks - stars: individual: HD 163296 - submillimeter: stars - submillimeter: stars

VizieR on-line data: <Available at CDS (J/A+A/606/A125): list.dat fits/*>

Simbad objects: 9

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Number of rows : 9

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2020
#notes
1 V* DM Tau Or* 04 33 48.7335659850 +18 10 09.974471722 14.30 14.82 14.00     M2Ve 510 0
2 EM* LkCa 15 Or* 04 39 17.7912813350 +22 21 03.387667491   13.01 12.03 11.61   K5:Ve 552 1
3 HD 31648 Ae* 04 58 46.2654165113 +29 50 36.990341242 7.84 7.78 7.62 7.76 7.43 A5Vep 394 0
4 V* TW Hya TT* 11 01 51.9054298616 -34 42 17.031550898   11.94 10.50 10.626 9.18 K6Ve 1532 1
5 THA 15-12 Or* 15 56 09.2067120748 -37 56 06.126159332   13.12 11.93 11.45   M0e 245 0
6 IRAS 16293-2422 cor 16 32 22.56 -24 28 31.8           ~ 1035 1
7 EM* AS 209 Or* 16 49 15.3035547820 -14 22 08.642015783   12.62 11.28     K4Ve 233 0
8 QSO B1730-130 QSO 17 33 02.70578476 -13 04 49.5481484   18 18.5 18.78 17.39 ~ 983 1
9 HD 163296 Ae* 17 56 21.2882188601 -21 57 21.872343282 7.00 6.93 6.85 6.86 6.67 A1Vep 802 0

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2020.07.10-02:19:25

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