Decrease of the organic deuteration during the evolution of Sun-like protostars: the case of SVS13-A
arXiv:1701.08656 · doi:10.1093/mnras/stx252
Abstract
We present the results of formaldehyde and methanol deuteration measurements towards the Class I low-mass protostar SVS13-A, in the framework of the IRAM 30-m ASAI (Astrochemical Surveys At IRAM) project. We detected emission lines of formaldehyde, methanol, and their deuterated forms (HDCO, D2CO, CHD2OH, CH3OD) with Eup up to 276 K. The formaldehyde analysis indicates Tkin = 15 - 30 K, n (H2) >= 10^6 cm^-3, and a size of about 1200 AU suggesting an origin in the protostellar envelope. For methanol we find two components: (i) a high temperature (Tkin = 80 K) and very dense (> 10^8 cm^-3}) gas from a hot corino (radius about 35 AU), and (ii) a colder Tkin <= 70 K) and more extended (radius about 350 AU) region. The deuterium fractionation is 9 10^-2 for HDCO, 4 10^-3 for D2CO, and 2 - 7 10^-3 for CH2DOH, up to two orders of magnitude lower than the values measured in Class 0 sources. We derive also formaldehyde deuteration in the outflow: 4 10^-3, in agreement with what found in the L1157-B1 protostellar shock. Finally, we estimate [CH2DOH]/[CH3OD] about 2. The decrease of deuteration in the Class I source SVS13-A with respect to Class 0 sources can be explained by gas-phase processes. Alternatively, a lower deuteration could be the effect of a gradual collapse of less deuterated external shells of the protostellar evelope. The present measurements fill in the gap between prestellar cores and protoplanetary disks in the context of organics deuteration measurements.
MNRASS, in press, 13 pages, 10 figures
References in corpus (26)
- The Spitzer c2d Legacy Results: Star Formation Rates and Efficiencies; Evolution and Lifetimes
- Our astrochemical heritage
- Unveiling the Circumstellar Envelope and Disk: A Sub-Arcsecond Survey of Circumstellar Structures
- The VLA Nascent Disk and Multiplicity Survey of Perseus Protostars (VANDAM). II. Multiplicity of Protostars in the Perseus Molecular Cloud
- First detection of triply-deuterated methanol
- Astrometry of Water Maser Sources in Nearby Molecular Clouds with VERA - II. SVS 13 in NGC 1333
- Detection of doubly-deuterated methanol in the solar-type protostar IRAS16293-2422
- The chemical history of molecules in circumstellar disks. I. Ices
- Exploring Molecular Complexity with ALMA (EMoCA): Deuterated complex organic molecules in Sagittarius B2(N2)
- CO Depletion and Deuterium Fractionation in Prestellar Cores
- The importance of the ortho:para H2 ratio for the deuteration of molecules during pre-protostellar collapse
- Weeds: a CLASS extension for the analysis of millimeter and sub-millimeter spectral surveys
- Testing grain surface chemistry : a survey of deuterated formaldehyde and methanol in low-mass Class 0 protostars
- Shedding light on the formation of the pre-biotic molecule formamide with ASAI
- Multilayer formation and evaporation of deuterated ices in prestellar and protostellar cores
- Deuterated methanol in the pre-stellar core L1544
- Formaldehyde and methanol deuteration in protostars: fossiles from a past fast high density pre-collapse phase
- Water ice deuteration: a tracer of the chemical history of protostars
- Theoretical HDO emission from low-mass protostellar envelopes
- Detection of DCO+ in a circumstellar disk
- Deuterated molecules in DM Tau: DCO+, but no HDO
- IRAM-PdBI Observations of Binary Protostars I: The Hierarchical System SVS13 in NGC1333
- Evidence for Multiple Pathways to Deuterium Enhancements in Protoplanetary Disks
- Detection of a hot core in the intermediate-mass (IM) Class 0 protostar NGC 7129--FIRS2
- An Unbiased Spectral Line Survey toward R CrA IRS7B in the 345 GHz Window with ASTE
- Hot and dense water in the inner 25 AU of SVS13-A
Cited by in corpus (37)
- Seeds Of Life In Space (SOLIS): The organic composition diversity at 300--1000 au scale in Solar-type star forming regions
- Astrochemical evolution along star formation: Overview of the IRAM Large Program ASAI
- The census of interstellar complex organic molecules in the Class I hot corino of SVS13-A
- First Abundance Measurement of Organic Molecules in the Atmosphere of HH 212 Protostellar Disk
- Mapping deuterated methanol toward L1544: I. Deuterium fraction and comparison with modeling
- FAUST I. The hot corino at the heart of the prototypical Class I protostar L1551 IRS5
- PRODIGE -- Envelope to Disk with NOEMA II. Small-scale temperature structure and a streamer feeding the SVS13A protobinary using CH3CN and DCN
- Prestellar grain-surface origins of deuterated methanol in comet 67P/Churyumov-Gerasimenko
- First Hot Corino detected around an Isolated Intermediate-Mass Protostar: Cep\,E-mm
- Deuterated methanol on Solar System scale around the HH212 protostar
- Organic molecules in the protoplanetary disk of DG Tau revealed by ALMA
- The two hot corinos of the SVS13-A protostellar binary system: counterposed siblings
- A Survey of CH2DOH Towards Starless and Prestellar Cores in the Taurus Molecular Cloud
- Chemical survey of Class I protostars with the IRAM-30m
- Successive deuteration in low-mass star-forming regions: the case of D-methanol (CHDOH) in IRAS 16293-2422
- ALMA Survey of Orion Planck Galactic Cold Clumps (ALMASOP): I. Detection of New Hot Corinos with ACA
- Importance of source structure on complex organics emission. I. Observations of CHOH from low-mass to high-mass protostars
- Methanol deuteration in high-mass protostars
- The SVS13-A Class I chemical complexity as revealed by S-bearing species. SOLIS XIII
- FAUST XVII: Super deuteration in the planet forming system IRS 63 where the streamer strikes the disk
- CHCN deuteration in the SVS13-A Class I hot-corino. SOLIS XV
- Deuterium and N fractionation in NH during the formation of a Sun-like star
- Linking the dust and chemical evolution: Taurus and Perseus -- New collisional rates for HCN, HNC, and their C, N, and H isotopologues
- PRODIGE -- Envelope to Disk with NOEMA III. The origin of complex organic molecule emission in SVS13A
- First detection of CHDOH towards pre-stellar cores
- Deuterated methanol toward NGC 7538-IRS1
- Nascent chemical complexity in prestellar core IRAS 16293E: complex organics and deuterated methanol
- Resolved Gas Temperatures and 12C/13C ratios in SVS13A from ALMA Observations of CH3CN and CH3-13-CN
- Observations and chemical modeling of the isotopologues of formaldehyde and the cations of formyl and protonated formaldehyde in the hot molecular core G331.512-0.103
- Gas phase Elemental abundances in Molecular cloudS (GEMS). IX. Deuterated compounds of H2S in starless cores
- The hot corino-like chemistry of four FUor-like protostars
- Hunting pre-stellar cores with APEX: overview
- Chemical complexity in star formation induced by stellar feedback: cores shock-formed by the supernova remnant W44
- Post-Outburst Chemistry in a Very Low-Luminosity Object: Peculiar High Abundance of Nitric Oxide
- Survival of Molecular Complexity under Recent Supernova Feedback: Detection of Hot Cores in RX J1713.7-3946
- The emergence of molecular complexity in star forming regions as seen with ASAI
- Singly- and doubly-deuterated formaldehyde in massive star-forming regions