J/A+AS/118/47 CO observations in spirals (Chini+, 1996)
Dust and CO emission in normal spirals. I. The data
Chini R., Kruegel E., Lemke R.
<Astron. Astrophys. Suppl. Ser. 118, 47 (1996)>
=1996A&AS..118...47C 1996A&AS..118...47C (SIMBAD/NED BibCode)
ADC_Keywords: Galaxies, radio ; CO ;
Keywords: galaxies: abundances - galaxies: interstellar matter -
galaxies: spiral - radio continuum: galaxies - radio lines: galaxies
Description:
We present 1300µm continuum observations and measurements of the
CO (1-0) and (2-1) emission from the inner regions of 98 normal
galaxies. The spatial resolution ranges from 11arcsec to 45arcsec.
The sources come from a complete FIR selected sample of 138 inactive
spirals with an optical diameter D25≤180arcsec.
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
table1 70 97 Dust emission in normal spirals
table2 75 108 CO emission in normal spirals
tables.tex 112 424 LaTeX version of the tables
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Byte-by-byte Description of file: table1
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Bytes Format Units Label Explanations
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1- 9 A9 --- Name Galaxy name
11- 12 I2 h RAh Right ascension 1950
14- 15 I2 min RAm Right ascension 1950
17- 20 F4.1 s RAs Right ascension 1950
22 A1 --- DE- Declination sign
23- 24 I2 deg DEd Declination 1950
26- 27 I2 arcmin DEm Declination 1950
29- 30 I2 arcsec DEs Declination 1950
32- 36 F5.1 Mpc Dist ? Distance
39- 42 F4.1 mJy S11 ? 1300um flux density whithin 11" area,
IRAM 30m telescope (MRT) observations
44- 47 F4.1 mJy e_S11 ? rms uncertainty on S11
50- 54 F5.1 mJy S24 ? 1300um flux density whithin 24" area,
Swedish ESO Submillimeter Telescope (SEST)
observations
57- 60 F4.1 mJy e_S24 ? rms uncertainty on S24
63- 65 I3 mJy S70 ? 1300um flux density whithin 70" area,
SEST observations
67- 70 F4.1 mJy e_S70 ? rms uncertainty on S70
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Byte-by-byte Description of file: table2
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Bytes Format Units Label Explanations
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1- 8 A8 --- Name Galaxy name
10 A1 --- n_Name A '*' indicates that the spectrum has been
fitted by two Gaussians, and that the
followed data are from the second Gaussian
12- 15 I4 km/s Vc1 ? CO(1-0) MRT (24") central velocity
17- 19 I3 km/s dVc1 ? CO(1-0) MRT (24") line width
21- 23 I3 mK Tmb1 ? CO(1-0) MRT (24") temperature
27- 30 I4 km/s Vc2 ? CO(1-0) SEST (45") central velocity
32- 34 I3 km/s dVc2 ? CO(1-0) SEST (45") line width
36- 38 I3 mK Tmb2 ? CO(1-0) SEST (45") temperature
40- 43 I4 km/s Vc3 ? CO(2-1) MRT (12") central velocity
45- 47 I3 km/s dVc3 ? CO(2-1) MRT (12") line width
49- 51 I3 mK Tmb3 ? CO(2-1) MRT (12") temperature
53- 56 I4 km/s Vc4 ? CO(2-1) SEST (24") central velocity
58- 60 I3 km/s dVc4 ? CO(2-1) SEST (24") line width
62- 64 I3 mK Tmb4 ? CO(2-1) SEST (24") temperature
67- 70 F4.2 --- I24" ? I(2-1)/(1-0) integrated intensities ratio
with the (1-0) lines coming from the 30m
telescope and the other from SEST
72- 75 F4.2 --- ISEST ? I(2-1)/(1-0) integrated intensities ratio
observations refers to 45" in the (1-0)
transition and 24" in (2-1)
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(End) Patricia Bauer [CDS] 02-Apr-1996