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Table D.1

Molecular line width in comets in m s−1.

46P:FWHM Hale-Bopp V HM (a) C/2014 Q2 V HM (a)

Molecule (b) December 2018 February 1997 (c) April 1997 May 1997 January 2015
H2S 1050 ± 30 − 920 ± 70 − 870 ± 40 − 820 ± 40 − 740 ± 85
SO2 − 1055 ± 47 − 962 ± 40 − 1300 ± 250
H2CS − 760 ± 190
H2CO 1260 ± 100 − 1150 ± 40 − 1030 ± 57 − 965 ± 8 − 855 ± 17
SO − 1103 ± 37 − 915 ± 45 − 780 ± 115
HCOOH − 980 ± 50 − 890 ± 70 − 750 ± 120
CH3CHO 1230 ± 240 − 1045 ± 149 − 840 ± 70 − 830 ± 40
NH2CHO 1200 ± 198 − 890 ± 56 − 542 ± 165 − 900 ± 70
OCS − 1020 ± 45 − 890 ± 90 − 840 ± 90
HC3N − 1350 ± 234 − 1120 ± 20 − 1060 ± 60 − 670 ± 140
(CH2OH)2 1105 ± 186 − 1030 ± 200 − 770 ± 60
HNCO − 1260 ± 62 − 980 ± 110 − 830 ± 40
CS 1200 ± 142 − 1120 ± 40 − 1035 ± 7 − 980 ± 30 − 880 ± 10
C2H5OH 1293 ± 348 − 709 ± 437 − 770 ± 100
CH2OHCHO − 1020 ± 230
HCN 1165 ± 10 − 1230 ± 20 − 1050 ± 70 − 880 ± 5
HNC 720 ± 195 − 1230 ± 15 − 1200 ± 110 − 1016 ± 108
CH3OH 1175 ± 20 − 1320 ± 30 − 1058 ± 38 − 960 ± 30 − 867 ± 4
CH3CN 1030 ± 118 − 1014 ± 144 − 1000 ± 80 − 760 ± 50
CO − 1270 ± 60 − 1150 ± 50 − 960 ± 90 − 810 ± 70

Notes. (a) Negative VHM values correspond to the blueshifted side of the line (due to a sun-ward jet). (b) Ordered by ~ increasing lifetime. (c)Data obtained mostly with the 10.4 m Caltech Submillimeter Observatory or Plateau Bure 15 m antennas and a 24 ± 4′′ beamsize. April–May data were obtained with the IRAM 30 m and a 12 ± 3′′ beamsize. (d)CS, HNC, and more notably SO and H2CO (which have a much shorter daughter/parent scale length ratio) are daughter molecules. Their scale length can be much longer than expected for a parent molecule.

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