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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