Cardiff University | Prifysgol Caerdydd ORCA
Online Research @ Cardiff 
WelshClear Cookie - decide language by browser settings

Deuterated formaldehyde in rho Ophiuchi A

Bergman, P., Parise, Berengere, Liseau, R. and Larsson, B. 2011. Deuterated formaldehyde in rho Ophiuchi A. Astronomy and Astrophysics 527 , A39. 10.1051/0004-6361/201015012

[img]
Preview
PDF - Published Version
Download (1MB) | Preview

Abstract

Context. Formaldehyde is an organic molecule that is abundant in the interstellar medium. High deuterium fractionation is a common feature in low-mass star-forming regions. Observing several isotopologues of molecules is an excellent tool for understanding the formation paths of the molecules. Aims. We seek an understanding of how the various deuterated isotopologues of formaldehyde are formed in the dense regions of low-mass star formation. More specifically, we adress the question of how the very high deuteration levels (several orders of magnitude above the cosmic D/H ratio) can occur using H2CO data of the nearby ρ Oph A molecular cloud. Methods. From mapping observations of H2CO, HDCO, and D2CO, we have determined how the degree of deuterium fractionation changes over the central 3′ × 3′ region of ρ Oph A. The multi-transition data of the various H2CO isotopologues, as well as from other molecules (e.g., CH3OH and N2D + ) present in the observed bands, were analysed using both the standard type rotation diagram analysis and, in selected cases, a more elaborate method of solving the radiative transfer for optically thick emission. In addition to molecular column densities, the analysis also estimates the kinetic temperature and H2 density. Results. Toward the SM1 core in ρ Oph A, the H2CO deuterium fractionation is very high. In fact, the observed D2CO/HDCO ratio is 1.34 ± 0.19, while the HDCO/H2CO ratio is 0.107 ± 0.015. This is the first time, to our knowledge, that the D2CO/HDCO abundance ratio is observed to be greater than 1. The kinetic temperature is in the range 20−30 K in the cores of ρ Oph A, and the H2 density is (6−10) × 105 cm-3. We estimate that the total H2 column density toward the deuterium peak is (1−4) × 1023 cm-2. As depleted gas-phase chemistry is not adequate, we suggest that grain chemistry, possibly due to abstraction and exchange reactions along the reaction chain H2CO → HDCO → D2CO, is at work to produce the very high deuterium levels observed.

Item Type: Article
Status: Published
Schools: Physics and Astronomy
Subjects: Q Science > QB Astronomy
Uncontrolled Keywords: astrochemistry ; ISM: abundances ; ISM: clouds ; ISM: individual objects:ρ Ophiuchi A ; ISM: molecules
Additional Information: Pdf uploaded in accordance with publisher's policy at http://www.sherpa.ac.uk/romeo/issn/0004-6361/ (accessed 16/04/2014)
Publisher: EDP Sciences
ISSN: 0004-6361
Date of First Compliant Deposit: 30 March 2016
Last Modified: 19 Mar 2016 09:40
URI: http://orca-mwe.cf.ac.uk/id/eprint/52780

Citation Data

Cited 29 times in Google Scholar. View in Google Scholar

Cited 43 times in Scopus. View in Scopus. Powered By Scopus® Data

Actions (repository staff only)

Edit Item Edit Item

Downloads

Downloads per month over past year

View more statistics