J/A+A/279/541 Sub-mm observations of SNR IC 443 (van Dishoeck+ 1993)
Submillimeter observations of the shocked molecular gas associated with
the supernova remnant IC 443
Van Dishoeck E.F., Jansen D.J., Phillips T.G.
<Astron. Astrophys. 279, 541 (1993)>
=1993A&A...279..541V 1993A&A...279..541V
ADC_Keywords: Supernova remnants ; Radio lines
Keywords: ISM : molecules - ISM : supernova remnants -
ISM: individual objects: IC 443 - shock waves -
radio lines : interstellar
Objects:
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RA (2000) DE Designation(s)
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06 16.0 +22 24 IC 443 = SNR 189.0+03.0 = 3C 157
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File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
table1 67 57 Observations and fits of IC 443 G I
table2 67 23 Observations and fits of IC 443 G II
table3 67 50 Observations and fits of IC 443 B
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Byte-by-byte Description of file: table2 table1 table3
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Bytes Format Units Label Explanations
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1- 7 A7 --- Species Ion or molecule name
12- 22 A11 --- Transit Transition levels upper-lower
24- 29 I6 MHz Freq Frequency
31 A1 --- l_T(MB) '<' if T(MB) is an upper limit
(upper limits are 2 sigma values in 1 MHz
bandwidth)
32- 36 F5.2 K T(MB) ?Main beam temperature
40- 44 F5.1 km/s V(LSR) ?Velocity
47- 50 F4.1 km/s DV ?FWHM of line
53- 57 F5.1 K.km/s W ?Main beam temperature integrated over profile
59 A1 --- Note Remark (see below)
61- 68 A8 --- Obs Telescope and Year of observation
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Individual Note to table1:
a: upper limits are 2 sigma values in 1 MHz bandwidth
Preshock and shocked emission cannot be distinguished; about 20 % of
the integrated emission is estimated to be due to the preshocked gas.
Individual Note to table3:
DV is kept fixed at 12, 20 and 20 km/s in the fit to those
profiles that show multiple components.
(End) Francois Ochsenbein [CDS] 20-Jul-1993