2010A&A...517A..17D


Query : 2010A&A...517A..17D

2010A&A...517A..17D - Astronomy and Astrophysics, volume 517A17-17 (2010/7-1)

TIMASSS: the IRAS 16293-2422 millimeter and submillimeter spectral survey: tentative detection of deuterated methyl formate (DCOOCH3).

DEMYK K., BOTTINELLI S., CAUX E., VASTEL C., CECCARELLI C., KAHANE C. and CASTETS A.

Abstract (from CDS):

High deuterium fractionation is observed in various types of environments such as prestellar cores, hot cores, and hot corinos. It has proven to be an efficient probe for studying the physical and chemical conditions of these environments. The study of the deuteration of different molecules helps us to understand their formation. This is especially interesting for complex molecules like methanol and bigger molecules for which it may allow differentiation of gas-phase and solid-state formation pathways. Methanol exhibits a high deuterium fractionation in hot corinos. Since CH3OH is thought to be a precursor of methyl formate we expect that deuterated methyl formate is produced in such environments. We searched for the singly-deuterated isotopologue of methyl formate, DCOOCH3, in IRAS 16293-2422, a hot corino well-known for its high degree of methanol deuteration. We used the IRAM/JCMT unbiased spectral survey of IRAS 16293-2422, which allowed us to search for the DCOOCH3 rotational transitions within the survey spectral range (80-280GHz, 328-366GHz). The expected emission of deuterated methyl formate is modelled at LTE and compared with the observations. We have tentatively detected DCOOCH3 in the protostar IRAS 16293-2422. We assign eight lines detected in the IRAM survey to DCOOCH3. Three of these lines are affected by blending problems, and one is affected by calibration uncertainties; nevertheless, the LTE emission model is compatible with the observations. A simple LTE modelling of the two cores in IRAS 16293-2422, based on a previous interferometric study of HCOOCH3, allows us to estimate the amount of DCOOCH3 in IRAS 16293-2422. Adopting an excitation temperature of 100K and a source size of 2"and 1.5" for the A and B cores, respectively, we find that NA,DCOOCH3=NB, DCOOCH3∼6x1014cm–2. The derived deuterium fractionation is ∼15%, consistent with values for other deuterated species in this source and much greater than expected from the deuterium cosmic abundance. If its tentative detection is confirmed, DCOOCH3 should now be considered in theoretical models that study complex molecule formation and their deuteration mechanisms. Experimental work is also needed to investigate the different chemical routes leading to the formation of deuterated methyl formate.

Abstract Copyright: ∼

Journal keyword(s): line: identification - methods: observational - ISM: molecules - ISM: abundances - ISM: individual objects: IRAS 16293-2422 - radio lines: ISM

Simbad objects: 1

goto Full paper

goto View the references in ADS

Number of rows : 1
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 IRAS 16293-2422 cor 16 32 22.56 -24 28 31.8           ~ 1357 1

Query : 2010A&A...517A..17D

Basic data :
IRAS 16293-2422 -- Dense Core
Other object types:
otypes_help
smm (2008ApJ,JCMTLSG,...), IR (2013ApJS,HGBS,...), MIR (SSTc2d,WISEA,...), Y*O (2015MNRAS,[EES2009]), Y*? (2015ApJS,[HL2013]), mm (2009ApJ,[YEE2006]), cor (2020A&A), PoC ([FST86])
ICRS coord. (ep=J2000) :
16 32 22.56 -24 28 31.8 (Infrared) [ 300 300 90 ] C 2009ApJ...692..973E
FK4 coord. (ep=B1950 eq=1950) :
16 29 20.71 -24 22 11.7 [ 300 300 90 ]
Gal coord. (ep=J2000) :
353.93571 +15.84097 [ 300 300 90 ]
Angular size (arcmin):
0.35 0.13 136 (FIR) C 2020A&A...638A..74L
SIMBAD within arcmin
Overlay Simbad points in this preview
Back
All CDSPortal (CDSPortal)

Send to sendBySAMP sendBySAMP

sedIcon
within arcsec sed-help-icon
notes:


Hierarchy : number of linked objects
whatever the membership probability is (see description here ) :

: 1
: 2
: 2355 Display criteria :

Identifiers (18) :
An access of full data is available using the icon Vizier near the identifier of the catalogue

HGBS J163223.1-242836 NAME IRAS 16293 WISE J163222.62-242833.6 [JJK2008] SMM J163223-24284
IRAS 16293-2422 NAME rho Oph East [EDJ2009] 1008 [NWA2006] SMM 20
JCMTLSG J163222.6-242833 SSTc2d J163222.6-242832 [EES2009] Oph-emb 2 [YEE2006] 37
JCMTSE J163222.8-242837 SSTc2d J163222.6-242831 [FST86] rho Oph E
JCMTSF J163222.8-242837 WISEA J163222.60-242833.6 [HL2013] 248.09427-24.47550

References (1357 between 1850 and 2026) (Total 1357)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
Follow new references on this object
                Reference summaries :

                from: to:

                 or select by : (not exhaustive, explanation here)


Observing logs

Herschel : 27    ISO : 23   

   


External archives :

Data at NED - NASA/IPAC Extragalactic Database : IRAS 16293-2422

Link by name to the catalogue in VizieR :

IRAS 16293-2422 WISEA J163222.60-242833.6 WISE J163222.62-242833.6

Search by coordinates in Vizier (radius: 5 arcsec)


Annotations :
Annotations allow a user to add a note or report an error concerning the astronomical object and its data. It requires registration to post a note. See description .
Please, have a look at Best practices. The list of all annotations to SIMBAD objects can be found here .

The annotation server is currently not available. Sorry for any inconvenience


To bookmark this query, right click on this link: simbad:objects in 2010A&A...517A..17D and select 'bookmark this link' or equivalent in the popup menu