2013A&A...559A..47B


C.D.S. - SIMBAD4 rel 1.7 - 2020.07.11CEST20:05:58

2013A&A...559A..47B - Astronomy and Astrophysics, volume 559A, 47-47 (2013/11-1)

Complex organic molecules in the interstellar medium: IRAM 30 m line survey of Sagittarius B2(N) and (M).

BELLOCHE A., MUELLER H.S.P., MENTEN K.M., SCHILKE P. and COMITO C.

Abstract (from CDS):

The discovery of amino acids in meteorites fallen to Earth and the detection of glycine, the simplest of them, in samples returned from a comet to Earth strongly suggest that the chemistry of the interstellar medium is capable of producing such complex organic molecules and that they may be widespread in our Galaxy. Our goal is to investigate the degree of chemical complexity that can be reached in the interstellar medium, in particular in dense star-forming regions. We performed an unbiased, spectral line survey toward Sgr B2(N) and (M), two regions where high-mass stars are formed, with the IRAM 30m telescope in the 3mm atmospheric transmission window. Partial surveys at 2 and 1.3mm were performed in parallel. The spectra were analyzed with a simple radiative transfer model that assumes local thermodynamic equilibrium but takes optical depth effects into account. About 3675 and 945 spectral lines with a peak signal-to-noise ratio higher than 4 are detected at 3mm toward Sgr B2(N) and (M), i.e. about 102 and 26 lines per GHz, respectively. This represents an increase by about a factor of two over previous surveys of Sgr B2. About 70% and 47% of the lines detected toward Sgr B2(N) and (M) are identified and assigned to 56 and 46 distinct molecules as well as to 66 and 54 less abundant isotopologues of these molecules, respectively. In addition, we report the detection of transitions from 59 and 24 catalog entries corresponding to vibrationally or torsionally excited states of some of these molecules, respectively, up to a vibration energy of 1400cm–1 (2000K). Excitation temperatures and column densities were derived for each species but should be used with caution. The rotation temperatures of the detected complex molecules typically range from ∼50 to 200K. Among the detected molecules, aminoacetonitrile, n-propyl cyanide, and ethyl formate were reported for the first time in space based on this survey, as were five rare isotopologues of vinyl cyanide, cyanoacetylene, and hydrogen cyanide. We also report the detection of transitions from within twelve new vibrationally or torsionally excited states of known molecules. Absorption features produced by diffuse clouds along the line of sight are detected in transitions with low rotation quantum numbers of many simple molecules and are modeled with ∼30-40 velocity components with typical linewidths of ∼3-5km/s. Although the large number of unidentified lines may still allow future identification of new molecules, we expect most of these lines to belong to vibrationally or torsionally excited states or to rare isotopologues of known molecules for which spectroscopic predictions are currently missing. Significant progress in extending the inventory of complex organic molecules in Sgr B2(N) and deriving tighter constraints on their location, origin, and abundance is expected in the near future thanks to an ongoing spectral line survey at 3mm with ALMA in its cycles 0 and 1. The present single-dish survey will serve as a solid basis for the line identification and analysis of such an interferometric survey.

Abstract Copyright:

Journal keyword(s): astrobiology - astrochemistry - line: identification - stars: formation - ISM: individual objects: Sagittarius B2 - ISM: molecules

VizieR on-line data: <Available at CDS (J/A+A/559/A47): b2n_ids1.dat b2n_ids2.dat b2n_ids3.dat b2n_spec.dat b2m_ids1.dat b2m_ids2.dat b2m_ids3.dat b2m_spec.dat fits/*>

Errata: + corrigendum vol. 561, p. C1 (2014)

Simbad objects: 20

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Number of rows : 20

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2020
#notes
1 TMC-1 MoC 04 41 45.9 +25 41 27           ~ 1359 0
2 RAFGL 618 pA* 04 42 53.6245215366 +36 06 53.397219192   16.32   12.59   C-rich 954 0
3 NAME Orion-KL SFR 05 35 14.16 -05 22 21.5           ~ 2001 1
4 IRC +10216 C* 09 47 57.40632 +13 16 43.5648     10.96     C9,5e 2134 0
5 NAME Crux Arm PoG 12 30 -60.0           ~ 82 0
6 GAL 327.30-00.60 HII 15 53 05.0 -54 35 24           ~ 122 0
7 NAME Gal Center reg 17 45 40.04 -29 00 28.1           ~ 11542 0
8 NAME Sgr B MoC 17 47 02 -28 25.4           ~ 189 0
9 NAME Sgr B2 (North) Rad 17 47 20.2 -28 22 21           ~ 514 1
10 NAME Sgr B2 MoC 17 47 20.4 -28 23 07           ~ 1909 1
11 NAME Sgr B2 Main Rad 17 47 20.5 -28 23 06           ~ 331 1
12 NAME Sgr B2 (OH) MoC 17 47 20.8 -28 23 32           ~ 80 0
13 GAL 010.47+00.03 HII 18 08 38.4 -19 51 52           ~ 109 0
14 W 31c HII 18 10 29.1 -19 56 05           ~ 301 0
15 OH 34.26 +0.15 SFR 18 53 18.54 +01 14 57.9           ~ 460 0
16 NAME Sgr Arm PoG 19 00 -30.0           ~ 523 1
17 W 51e1 Rad 19 23 43.77 +14 30 25.9           ~ 115 0
18 W 51e2 Rad 19 23 43.90 +14 30 34.8           ~ 180 0
19 HH 375 Y*O 20 39 06.2 +68 02 15           ~ 158 0
20 LDN 1157 DNe 20 39 06.4 +68 02 13           ~ 484 0

    Equat.    Gal    SGal    Ecl

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2020.07.11-20:05:58

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