Highlight
Free Access

Table 6

Molecular line emission from the EDEa.

Line Apertureb S FWZPc I
(′′) (Jy) (km s−1) (Jy km s−1)
C18O(2–1)d 3 1.4 12
SiO(5–4) 3 0.38 22.3 4.5
CS(4–3) 32 0.35 12.6 5.0
13CS(5–4) 3 0.11 18.0 1.9
SO(55−44) 3 0.30 30.2 5.4
SO(56−45) 3 0.18 31.4 4.0
SO(65−54)e 24 0.08 20.0 1.7
34SO(56−45) 3 0.08: 28: 1.5
SO2(422−313) 3 0.035 35: 0.81
o-H2S(110−101) 37 1.9 15.4 19
p-H2S(220−211) 3 2.8 17.9 23
28 2.4 15.3 17
o-H2S(330−321) 21 2.8 12.7 17
p-H2S(202−111) 9 5: 6: 25:
         
o-HS(110−101)f 37 12
         
p-HS(220−211)f 3 3.4
         
p-HS(202−111)f 9 24:
         
o-HS(110−101) 37 1.6 16.6 12
         
p-HS(220−211) 3 1.2 15.0 6.7
         
p-HS(202−111) 9 5: 6: 12

Notes. (a) See Sect. 3 for a discussion of the flux uncertainties. (b)Centred on the continuum peak. (c)FWZP of the line within the given aperture at 1.5 km s−1 resolution. (d)Data obtained within a velocity range of 20 km s−1 centred on the systemic velocity. (e)This is based on APEX data and the split into emission from the CCS and EDE components obtained using Gaussian decomposition is uncertain. (f) The integrated intensity of the sum of the hyperfine components.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.