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J/A+AS/126/3 CO and HI in interacting galaxies (Horellou+ 1997)
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CO and HI in a southern sample of interacting galaxies. I. The data
Horellou C., Booth R.
<Astron. Astrophys. Suppl. Ser. 126, 3 (1997)>
=1997A&AS..126....3H (SIMBAD/NED BibCode)
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ADC_Keywords: Radio lines ; Galaxies, spectra ; H I data ; CO
Keywords: galaxies: interaction - galaxies: ISM - galaxies: evolution -
radio lines: galaxies
Abstract:
Using SEST, the Parkes antenna and the Australia Telescope Compact
Array, we have made a survey of the ^12^CO(1-0) and HI emission of an
optically-selected sample of =~60 southern interacting and merging
galaxies. In this paper we present the data and determine global
masses of neutral gas (in molecular and atomic form) for the observed
galaxies. We have detected HI in 26 systems and found that
these galaxies have less than 15% of their gas in molecular form.
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
table1.dat 83 75 Galaxy Characteristics
table3.dat 85 66 HI and CO observational results
fig3p1.ps 81 5609 Optical images, HI and CO spectra
fig3p2.ps 81 10946 Figure 3 continued
fig3p3.ps 81 5779 Figure 3 continued
fig3p4.ps 81 28946 Figure 3 continued
fig3p5.ps 81 5255 Figure 3 continued
fig3p6.ps 81 14320 Figure 3 continued
fig3p7.ps 81 7357 Figure 3 continued
fig3p8.ps 81 5632 Figure 3 continued
fig3p9.ps 81 4176 Figure 3 continued
fig3p10.ps 81 8982 Figure 3 continued
fig3p11.ps 81 5876 Figure 3 continued
fig3p12.ps 81 7130 Figure 3 continued
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Byte-by-byte Description of file: table1.dat
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Bytes Format Units Label Explanations
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1- 6 A6 --- Name Source name
7 A1 --- Note [a-g] Note about individual galaxies (1)
9- 18 A10 --- FileName Name of postscript figure file containing
this galaxy (in this directory)
20- 31 A12 --- Galaxy Galaxy name (from ESO survey)
33- 34 I2 h RAh Right Ascension 1950 (hours)
36- 37 I2 min RAm Right Ascension 1950 (minutes)
39- 42 F4.1 s RAs Right Ascension 1950 (seconds)
44 A1 --- DE- Declination 1950 (sign)
45- 46 I2 deg DEd Declination 1950 (degrees)
48- 49 I2 arcmin DEm Declination 1950 (minutes)
51- 52 I2 arcsec DEs Declination 1950 (seconds)
55- 59 I5 km/s Vhel ? Heliocentric velocity
61- 67 A7 --- MType Morphological Type
70- 73 F4.2 [0.1arcmin] logD25 ? Diameter at 25mag/arcsec2 (log scale)
75- 83 A9 --- OtherName Other designation of the Galaxy
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Note (1):
a : JB01 has an uncertainty in position of 30x30arcsec.
NED gives also a radio velocity of 10079km/s
b : JB06_2 has an uncertainty in position of 30x30arcsec
c : JB14_2 other authors give Vhel=6321km/s
d : JB29_1 has an uncertainty in position of 30x30arcsec
e : JB33 has an uncertainty in position of 9x9arcsec
f : JB40 has an uncertainty in position of 5x5arcsec
g : JB56 HI line at Vhel=2600km/s towards JB56
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Byte-by-byte Description of file: table3.dat
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Bytes Format Units Label Explanations
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2- 5 A4 --- HIname Source name
8 A1 --- Note [abdn] Note on source (1)
9 A1 --- posFlag [*] Flag for uncertain (30x30") position
11- 15 I5 km/s vHI ? HI velocity
18- 20 I3 km/s DvHI ? HI velocity width
22 A1 --- l_SHI Limit flag on SHI
23- 26 F4.1 Jy.km/s SHI ? Integrated HI flux
28- 30 F3.1 Jy.km/s e_SHI ? Mean error on HI flux
32 A1 --- l_M(HI) Limit flag on M(HI)
33- 36 F4.1 10+9solMass M(HI) ? Derived HI mass
39- 44 A6 --- Intrum Instrument used (Parkes or Australian
Telescope Compact Array)
49- 54 A6 --- Name Source name, as in table1
55 A1 --- Note(CO) [n] 'n' if not observed
56- 60 I5 km/s vCO ? CO velocity, observed at SEST telescope
at ESO-La Silla.
63- 65 I3 km/s DvCO ? CO velocity width
67 A1 --- l_SCO Limit flag on SCO
68- 71 F4.2 K.km/s SCO ? Integrated antenna temperature
73- 76 F4.2 K.km/s e_SCO ? Mean error on SCO
80 A1 --- l_M(H2) [*<] Limit flag on M(H2) ('*' stands
for tentative value)
81- 85 F5.1 10+8solMass M(H2) ? Mass of H2 derived from CO data.
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Note (1): the notes are
a = pointing made toward a position between galaxies JB11_1 and JB11_2
b = sources JB57 and JB58 observed together in HI
d = sources not separated in HI, but are separated in CO
n = not observed in HI
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Description of Figures (*.ps files):
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Column 1: contour and grey-scale pictures of the galaxies (ESO Digitized
Sky Survey). North is to the top, west to the right.
The scales on the axes are in arcsec.
Column 2: HI spectra. The spectral resolution is 6.6km/s. The units are km/s
on the X axis (radial velocities in the radio convention) and
Jy on the Y axis.
Column 3: CO spectra. The spectral resolution is 14.6km/s. The units are km/s
on the X axis (radial velocities in the radio convention) and
K on the Y axis (T_A_^*^).
When the two galaxies of a pair were observed, the two spectra are shown and
the name of the observed galaxy is given close to the corresponding spectrum.
The lower spectrum refers to the most southern galaxy on the
optical image, the upper one to the other.
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(End) Patricia Bauer [CDS] 02-May-1997