Please use this identifier to cite or link to this item: http://hdl.handle.net/10995/101809
Title: First ALMA maps of HCO, an important precursor of complex organic molecules, towards IRAS 16293-2422
Authors: Rivilla, V. M.
Beltrán, M. T.
Vasyunin, A.
Caselli, P.
Viti, S.
Fontani, F.
Cesaroni, R.
Issue Date: 2019
Publisher: Oxford University Press
Citation: First ALMA maps of HCO, an important precursor of complex organic molecules, towards IRAS 16293-2422 / V. M. Rivilla, M. T. Beltrán, A. Vasyunin, et al. — DOI 10.1093/mnras/sty3078 // Monthly Notices of the Royal Astronomical Society. — 2019. — Vol. 483. — Iss. 1. — P. 806-823.
Abstract: The formyl radical HCO has been proposed as the basic precursor of many complex organic molecules such as methanol (CH3OH) and glycolaldehyde (CH2OHCHO). Using ALMA, we have mapped, for the first time at high angular resolution (∼1 arcsec, ∼140 au), HCO towards the solar-type protostellar binary IRAS 16293-2422, where numerous complex organic molecules have been previously detected. We also detected several lines of the chemically related species H2CO, CH3OH, and CH2OHCHO. The observations revealed compact HCO emission arising from the two protostars. The line profiles also show redshifted absorption produced by foreground material of the circumbinary envelope that is infalling towards the protostars. Additionally, IRAM 30 m single-dish data revealed a more extended HCO component arising from the common circumbinary envelope. The comparison between the observed molecular abundances and our chemical model suggests that whereas the extended HCO from the envelope can be formed via gas-phase reactions during the cold collapse of the natal core, the HCO in the hot corinos surrounding the protostars is predominantly formed by the hydrogenation of CO on the surface of dust grains and subsequent thermal desorption during the protostellar phase. The derived abundance of HCO in the dust grains is high enough to produce efficiently more complex species such as H2CO, CH3OH, and CH2OHCHO by surface chemistry. We found that the main formation route of CH2OHCHO is the reaction between HCO and CH2OH. © 2018 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society
Keywords: ASTROCHEMISTRY
ISM: MOLECULES
LINE: IDENTIFICATION
MOLECULAR DATA
STARS: FORMATION
STARS: LOW-MASS
URI: http://hdl.handle.net/10995/101809
Access: info:eu-repo/semantics/openAccess
SCOPUS ID: 85062182277
PURE ID: 9189119
ISSN: 358711
DOI: 10.1093/mnras/sty3078
Appears in Collections:Научные публикации, проиндексированные в SCOPUS и WoS CC

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