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This article has an erratum: [erratum]

Issue
A&A
Volume 559, November 2013
Article Number A47
Number of page(s) 187
Section Interstellar and circumstellar matter
DOI https://doi.org/10.1051/0004-6361/201321096
Published online 08 November 2013

Online material

thumbnail Fig. 2

Spectrum obtained toward Sgr B2(N) in the 3 mm window with the IRAM 30 m telescope in main-beam temperature scale. The synthetic model is overlaid in green and its relevant lines are labeled in blue. The frequencies of the hydrogen recombination lines are indicated with a pink label. The position of the lines with a peak temperature higher than 2 K in the image band and possibly contaminating the spectrum are marked with a red label indicating their rest frequency and their peak temperature in K in the image band.

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thumbnail Fig. 3

Spectrum obtained toward Sgr B2(N) in the 2 mm window with the IRAM 30 m telescope in main-beam temperature scale. The synthetic model is overlaid in green and its relevant lines are labeled in blue. The frequencies of the hydrogen recombination lines are indicated with a pink label.

Open with DEXTER

thumbnail Fig. 4

Spectrum obtained toward Sgr B2(N) in the 1 mm window with the IRAM 30 m telescope in main-beam temperature scale. The synthetic model is overlaid in green and its relevant lines are labeled in blue. The frequencies of the hydrogen recombination lines are indicated with a pink label.

Open with DEXTER

thumbnail Fig. 5

Spectrum obtained toward Sgr B2(M) in the 3 mm window with the IRAM 30 m telescope in main-beam temperature scale. The synthetic model is overlaid in green and its relevant lines are labeled in blue. The frequencies of the hydrogen and helium recombination lines are indicated with a pink label. The position of the lines with a peak temperature higher than 2 K in the image band and possibly contaminating the spectrum are marked with a red label indicating their rest frequency and their peak temperature in K in the image band.

Open with DEXTER

thumbnail Fig. 6

Spectrum obtained toward Sgr B2(M) in the 2 mm window with the IRAM 30 m telescope in main-beam temperature scale. The synthetic model is overlaid in green and its relevant lines are labeled in blue. The frequencies of the hydrogen and helium recombination lines are indicated with a pink label.

Open with DEXTER

thumbnail Fig. 7

Spectrum obtained toward Sgr B2(M) in the 1 mm window with the IRAM 30 m telescope in main-beam temperature scale. The synthetic model is overlaid in green and its relevant lines are labeled in blue. The frequencies of the hydrogen and helium recombination lines are indicated with a pink label.

Open with DEXTER

Table 6

Parameters of our best-fit model of C2H3CN toward Sgr B2(N).

Table 7

Parameters of our best-fit model of C2H5CN toward Sgr B2(N).

Table 8

Parameters of our best-fit model of C2H5OCHO toward Sgr B2(N).

Table 9

Parameters of our best-fit model of C2H5OH toward Sgr B2(N).

Table 10

Parameters of our best-fit model of n-C3H7CN toward Sgr B2(N).

Table 11

Parameters of our best-fit model of c-C2H4O toward Sgr B2(N).

Table 12

Parameters of our best-fit model of c-C3H2 toward Sgr B2(N).

Table 13

Parameters of our best-fit model of CCH toward Sgr B2(N).

Table 14

Parameters of our best-fit model of CCS toward Sgr B2(N).

Table 15

Parameters of our best-fit model of CH2NH toward Sgr B2(N).

Table 16

Parameters of our best-fit model of aGg′-(CH2OH)2 toward Sgr B2(N).

Table 17

Parameters of our best-fit model of CH2(OH)CHO toward Sgr B2(N).

Table 18

Parameters of our best-fit model of CH3C3N toward Sgr B2(N).

Table 19

Parameters of our best-fit model of CH3CCH toward Sgr B2(N).

Table 20

Parameters of our best-fit model of CH3C(O)CH3 toward Sgr B2(N).

Table 21

Parameters of our best-fit model of CH3CHO toward Sgr B2(N).

Table 22

Parameters of our best-fit model of CH3CN toward Sgr B2(N).

Table 23

Parameters of our best-fit model of CH3C(O)NH2-A toward Sgr B2(N).

Table 24

Parameters of our best-fit model of CH3COOH toward Sgr B2(N).

Table 25

Parameters of our best-fit model of CH3NH2 toward Sgr B2(N).

Table 26

Parameters of our best-fit model of CH3OCH3 toward Sgr B2(N).

Table 27

Parameters of our best-fit model of CH3OCHO toward Sgr B2(N).

Table 28

Parameters of our best-fit model of CH3OH toward Sgr B2(N).

Table 29

Parameters of our best-fit model of CH3SH toward Sgr B2(N).

Table 30

Parameters of our best-fit model of CN toward Sgr B2(N).

Table 31

Parameters of our best-fit model of CO toward Sgr B2(N).

Table 32

Parameters of our best-fit model of CS toward Sgr B2(N).

Table 33

Parameters of our best-fit model of CH2CO toward Sgr B2(N).

Table 34

Parameters of our best-fit model of H2CO toward Sgr B2(N).

Table 35

Parameters of our best-fit model of H2CS toward Sgr B2(N).

Table 36

Parameters of our best-fit model of NH2CH2CN toward Sgr B2(N).

Table 37

Parameters of our best-fit model of H2S toward Sgr B2(N).

Table 38

Parameters of our best-fit model of HC3N toward Sgr B2(N).

Table 39

Parameters of our best-fit model of HCCNC toward Sgr B2(N).

Table 40

Parameters of our best-fit model of HCN toward Sgr B2(N).

Table 41

Parameters of our best-fit model of NH2CHO toward Sgr B2(N).

Table 42

Parameters of our best-fit model of HCO+ toward Sgr B2(N).

Table 43

Parameters of our best-fit model of HCS+ toward Sgr B2(N).

Table 44

Parameters of our best-fit model of HDO toward Sgr B2(N).

Table 45

Parameters of our best-fit model of HNC toward Sgr B2(N).

Table 46

Parameters of our best-fit model of HNCO toward Sgr B2(N).

Table 47

Parameters of our best-fit model of HNCS toward Sgr B2(N).

Table 48

Parameters of our best-fit model of HOCN toward Sgr B2(N).

Table 49

Parameters of our best-fit model of HOCO+ toward Sgr B2(N).

Table 50

Parameters of our best-fit model of HOC+ toward Sgr B2(N).

Table 51

Parameters of our best-fit model of HSCN toward Sgr B2(N).

Table 52

Parameters of our best-fit model of N2H+ toward Sgr B2(N).

Table 53

Parameters of our best-fit model of NH2CN toward Sgr B2(N).

Table 54

Parameters of our best-fit model of NH2D toward Sgr B2(N).

Table 55

Parameters of our best-fit model of NS toward Sgr B2(N).

Table 56

Parameters of our best-fit model of OCS toward Sgr B2(N).

Table 57

Parameters of our best-fit model of PN toward Sgr B2(N).

Table 58

Parameters of our best-fit model of SiO toward Sgr B2(N).

Table 59

Parameters of our best-fit model of SO2 toward Sgr B2(N).

Table 60

Parameters of our best-fit model of SO toward Sgr B2(N).

Table 61

Parameters of our best-fit model of t-HCOOH toward Sgr B2(N).

Table 62

Parameters of our best-fit model of C2H3CN toward Sgr B2(M).

Table 63

Parameters of our best-fit model of C2H5CN toward Sgr B2(M).

Table 64

Parameters of our best-fit model of C2H5OH toward Sgr B2(M).

Table 65

Parameters of our best-fit model of c-C3H2 toward Sgr B2(M).

Table 66

Parameters of our best-fit model of CCH toward Sgr B2(M).

Table 67

Parameters of our best-fit model of CCS toward Sgr B2(M).

Table 68

Parameters of our best-fit model of CH2NH toward Sgr B2(M).

Table 69

Parameters of our best-fit model of CH3C3N toward Sgr B2(M).

Table 70

Parameters of our best-fit model of CH3CCH toward Sgr B2(M).

Table 71

Parameters of our best-fit model of CH3C(O)CH3 toward Sgr B2(M).

Table 72

Parameters of our best-fit model of CH3CHO toward Sgr B2(M).

Table 73

Parameters of our best-fit model of CH3CN toward Sgr B2(M).

Table 74

Parameters of our best-fit model of CH3NH2 toward Sgr B2(M).

Table 75

Parameters of our best-fit model of CH3OCH3 toward Sgr B2(M).

Table 76

Parameters of our best-fit model of CH3OCHO toward Sgr B2(M).

Table 77

Parameters of our best-fit model of CH3OH toward Sgr B2(M).

Table 78

Parameters of our best-fit model of CH3SH toward Sgr B2(M).

Table 79

Parameters of our best-fit model of CN toward Sgr B2(M).

Table 80

Parameters of our best-fit model of CO toward Sgr B2(M).

Table 81

Parameters of our best-fit model of CS toward Sgr B2(M).

Table 82

Parameters of our best-fit model of CH2CO toward Sgr B2(M).

Table 83

Parameters of our best-fit model of H2CO toward Sgr B2(M).

Table 84

Parameters of our best-fit model of H2CS toward Sgr B2(M).

Table 85

Parameters of our best-fit model of H2S toward Sgr B2(M).

Table 86

Parameters of our best-fit model of HC3N toward Sgr B2(M).

Table 87

Parameters of our best-fit model of HC5N toward Sgr B2(M).

Table 88

Parameters of our best-fit model of HCN toward Sgr B2(M).

Table 89

Parameters of our best-fit model of NH2CHO toward Sgr B2(M).

Table 90

Parameters of our best-fit model of HCO+ toward Sgr B2(M).

Table 91

Parameters of our best-fit model of HCS+ toward Sgr B2(M).

Table 92

Parameters of our best-fit model of HDO toward Sgr B2(M).

Table 93

Parameters of our best-fit model of HNC toward Sgr B2(M).

Table 94

Parameters of our best-fit model of HNCO toward Sgr B2(M).

Table 95

Parameters of our best-fit model of HNCS toward Sgr B2(M).

Table 96

Parameters of our best-fit model of HOCN toward Sgr B2(M).

Table 97

Parameters of our best-fit model of HOCO+ toward Sgr B2(M).

Table 98

Parameters of our best-fit model of HOC+ toward Sgr B2(M).

Table 99

Parameters of our best-fit model of HSCN toward Sgr B2(M).

Table 100

Parameters of our best-fit model of N2H+ toward Sgr B2(M).

Table 101

Parameters of our best-fit model of NH2CN toward Sgr B2(M).

Table 102

Parameters of our best-fit model of NS toward Sgr B2(M).

Table 103

Parameters of our best-fit model of OCS toward Sgr B2(M).

Table 104

Parameters of our best-fit model of PN toward Sgr B2(M).

Table 105

Parameters of our best-fit model of SiO toward Sgr B2(M).

Table 106

Parameters of our best-fit model of SO2 toward Sgr B2(M).

Table 107

Parameters of our best-fit model of SO toward Sgr B2(M).


© ESO, 2013

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