First detection of cyanamide (NHCN) towards solar-type protostars
arXiv:1712.09548 · doi:10.1051/0004-6361/201732346
Abstract
Searches for the prebiotically-relevant cyanamide (NHCN) towards solar-type protostars have not been reported in the literature. We here present the first detection of this species in the warm gas surrounding two solar-type protostars, using data from the Atacama Large Millimeter/Submillimeter Array Protostellar Interferometric Line Survey (PILS) of IRAS 16293-2422 B and observations from the IRAM Plateau de Bure Interferometer of NGC1333 IRAS2A. We furthermore detect the deuterated and C isotopologues of NHCN towards IRAS 16293-2422 B. This is the first detection of NHDCN in the interstellar medium. Based on a local thermodynamic equilibrium analysis, we find that the deuteration of cyanamide ( 1.7%) is similar to that of formamide (NHCHO), which may suggest that these two molecules share NH as a common precursor. The NHCN/NHCHO abundance ratio is about 0.2 for IRAS 16293-2422 B and 0.02 for IRAS2A, which is comparable to the range of values found for Sgr B2. We explored the possible formation of NHCN on grains through the NH + CN reaction using the chemical model MAGICKAL. Grain-surface chemistry appears capable of reproducing the gas-phase abundance of NHCN with the correct choice of physical parameters.
arXiv commentAccepted in A&A
References in corpus (28)
- A KInetic Database for Astrochemistry (KIDA)
- Making other Earths: Dynamical Simulations of Terrestrial Planet Formation and Water Delivery
- A three-phase chemical model of hot cores: the formation of glycine
- Complex organic molecules in the interstellar medium: IRAM 30 m line survey of Sagittarius B2(N) and (M)
- The ALMA Protostellar Interferometric Line Survey (PILS): First results from an unbiased submillimeter wavelength line survey of the Class 0 protostellar binary IRAS 16293-2422 with ALMA
- Detection of the simplest sugar, glycolaldehyde, in a solar-type protostar with ALMA
- A 2 mm spectral line survey of the starburst galaxy NGC 253
- Constraining the abundances of complex organics in the inner regions of solar-type protostars
- Near-arcsecond resolution observations of the hot corino of the solar type protostar IRAS 16293-2422
- Gas phase formation of the prebiotic molecule formamide: insights from new quantum computations
- Rotational spectroscopy, tentative interstellar detection, and chemical modelling of N-methylformamide
- The ALMA-PILS survey: First detections of deuterated formamide and deuterated isocyanic acid in the interstellar medium
- Probing the inner 200 AU of low-mass protostars with the Submillimeter Array: Dust and organic molecules in NGC1333-IRAS2A
- The ALMA-PILS survey: First detections of ethylene oxide, acetone and propanal toward the low-mass protostar IRAS 16293-2422
- The ALMA-PILS survey: Detection of CHNCO toward the low-mass protostar IRAS 16293-2422 and laboratory constraints on its formation
- First results from the CALYPSO IRAM-PdBI survey. II. Resolving the hot corino in the Class 0 protostar NGC 1333-IRAS2A
- Simultaneous Hydrogenation and UV-photolysis Experiments of NO in CO-rich Interstellar Ice Analogues; linking HNCO, OCN-, NH2CHO and NH2OH
- A lambda = 1.3 mm and 2 mm molecular line survey towards M82
- Formation of the prebiotic molecule NHCHO on astronomical amorphous solid water surfaces: accurate tunneling rate calculations
- The ALMA Band 9 receiver - Design, construction, characterization, and first light
- The deuterium fractionation of water on solar-system scales in deeply-embedded low-mass protostars
- A spectral survey of the Star Forming Core of the Orion Nebula from 455 -- 507 GHz
- Detection of glycolaldehyde towards the solar-type protostar NGC1333 IRAS2A
- The ALMA-PILS survey: Formaldehyde deuteration in warm gas on small scales toward IRAS 16293-2422 B
- Detection of methylisocyanate (CH3NCO) in a solar-type protostar
- The ALMA-PILS survey: 3D modeling of the envelope, disks and dust filament of IRAS 16293-2422
- High DO/HDO ratio in the inner regions of the low-mass protostar NGC1333 IRAS2A
- Kinetic Monte Carlo simulations of the grain-surface back-diffusion effect
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- The ALMA-PILS survey: Isotopic composition of oxygen-containing complex organic molecules toward IRAS 16293-2422B
- Formation of complex organic molecules in hot molecular cores through nondiffusive grain-surface and ice-mantle chemistry
- Ingredients for Solar-like Systems: protostar IRAS 16293-2422 B versus comet 67P/Churyumov-Gerasimenko
- Complex organic molecules in the Galactic Centre: the N-bearing family
- Questioning the spatial origin of complex organic molecules in young protostars with the CALYPSO survey
- The ALMA-PILS survey: Complex nitriles towards IRAS 16293--2422
- The formation of peptide-like molecules on interstellar dust grains
- Complex organic molecules in low-mass protostars on Solar System scales -- II. Nitrogen-bearing species
- The family of amide molecules toward NGC 6334I
- The ALMA-PILS survey: First detection of nitrous acid (HONO) in the interstellar medium
- ALMA observations of the young protostellar system Barnard 1b: signatures of an incipient hot corino in B1b-S
- The ALMA-PILS survey: First detection of the unsaturated 3-carbon molecules Propenal (CHCHO) and Propylene (CH) towards IRAS 162932422 B
- Detection of the cyanomidyl radical (HNCN): a new interstellar species with the NCN backbone
- The ALMA-PILS survey: first detection of methyl isocyanide (CHNC) in a solar-type protostar
- The ALMA-PILS survey: First tentative detection of 3-hydroxypropenal (HOCHCHCHO) in the interstellar medium and chemical modeling of the CHO isomers
- The ALMA-PILS survey: Gas dynamics in IRAS 162932422 and the connection between its two protostars
- The prebiotic molecular inventory of Serpens SMM1 I. An investigation of the isomers CHNCO and HOCHCN
- Exploring molecular complexity with ALMA (EMoCA): Complex isocyanides in Sgr B2(N)
- Linking interstellar and cometary O: a deep search for OO in the solar-type protostar IRAS 16293--2422
- Successive deuteration in low-mass star-forming regions: the case of D-methanol (CHDOH) in IRAS 16293-2422
- New molecular species at redshift z=0.89
- The ALMA-PILS survey: propyne (CHCCH) in IRAS 162932422
- Rotational spectroscopy of mono-deuterated oxirane (-CHDO) and its detection towards IRAS 162932422 B
- Chemical models of adenine precursors cyanamide and carbodiimide in the interstellar medium
- Peptide Bonds in the Interstellar Medium: Facile Autocatalytic Formation from Nitriles on Water-Ice Grains
- Deuterated methyl mercaptan (CHSD): Laboratory rotational spectroscopy and search toward IRAS 16293-2422 B
- Millimetre-wave laboratory study of glycinamide and search for it with ALMA toward Sagittarius B2(N)
- The physical and chemical structure of Sagittarius B2, VIII. Full molecular line survey of hot cores
- Identification of interstellar cyanamide towards the hot molecular core G358.93-0.03 MM1
- The rotation-tunneling spectrum of 3-hydroxypropenal and confirmation of its detection toward IRAS 162932422 B
- Laboratory spectroscopic study of the N isotopomers of cyanamide, HNCN, and a search for them toward IRAS 162932422 B
- Millimetre-wave spectroscopy of 2-hydroxyprop-2-enal and an astronomical search with ALMA
- Observational studies on S-bearing molecules in massive star forming regions
- The hot corino-like chemistry of four FUor-like protostars
- Digging into the Massive Protostar S255IR NIRS3: A Study of Nitrogen-Bearing Molecules and Their Prebiotic Chemistry
- The Reaction between Atomic Carbon and Molecular Nitrogen as a Source of Cyanamide and Carbodiimide on Interstellar Ices