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J/PASJ/57/917  CO molecular clouds in southern Galactic Warp (Nakagawa+, 2005)

An unbiased search for molecular clouds in the southern Galactic Warp. Nakagawa M., Onishi T., Mizuno A., Fukui Y. <Publ. Astron. Soc. Jap., 57, 917-931 (2005)> =2005PASJ...57..917N
ADC_Keywords: Molecular clouds ; Radio lines Keywords: Galaxy: warp - ISM: abundances - ISM: clouds - radio lines: ISM Abstract: We made an unbiased search for molecular clouds in the Galactic Warp. This survey, covering an area of 56 square degrees at l=252° to 266° and b=-5° to -1°, revealed 70 molecular clouds, while only 6 clouds were previously known in this sector at R≳14.5kpc. Description: Observations were made in the J=1-012CO emission line at 2.6mm wavelength with the NANTEN telescope at the Las Campanas Observatory in Chile in the period from 2001 July to 2002 August. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 91 71 Observed properties and physical quantities of 70 CO clouds.
See also: J/PASJ/53/1081 : CO molecular clouds in Lupus (Tachihara+, 2001) J/PASJ/53/971 : CO catalog of LMC molecular clouds (Mizuno+, 2001) J/PASJ/56/313 : 13CO survey of Mon + CMa molecular clouds (Kim+, 2004) Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 2 I2 --- [NOM2005] Running number 4- 9 F6.2 deg GLON Position of observed points with maximum 12CO integrated intensities within CO clouds 11- 15 F5.2 deg GLAT Position of observed points with maximum 12CO integrated intensities within CO clouds 17- 21 F5.1 km/s VLSR ?=- LSR velocity is derived from a Gaussian fitting for the composite line profiles 23- 26 F4.1 kpc Dist ?=- Distance from the Sun 28- 31 F4.1 kpc R ?=- Distance from the galactic center (1) 33- 37 I5 pc Z ?=- Distance from the galactic plane (b=0, Z=Dist*tan(b)) 39- 44 F6.2 K.km/s IICO ?=- Total CO integrated intensity, ∫TR*dV, sum of integrated intensity of all observed positions in one cloud. 46- 48 F3.1 km/s dV ?=- Composite line width (from Gaussian fit to composite spectrum) 50- 53 F4.1 pc Rad ?=- Radius of the CO cloud 55- 58 F4.1 pc Radc ?=- Corrected radius of the CO cloud 60- 65 F6.1 pc2.K.km/s LCO ?=- Luminosity 67- 71 I5 solMass MCO ?=- Cloud mass derived from CO luminosity by using X=5.6x1020cm-2/(K.km/s) 73- 78 I6 solMass Mvir ?=- Virial mass = 210xRadcxdV2 80- 91 A12 --- Com Comment (2)
Note (1): Distance from the galactic center for b=0, assuming flat rotation curve (R=8.5kpc, V=220km/s). Note (2): Comments are as follows: cold IRAS = clouds which have a cold IRAS point source near the peak double peak = clouds which have multiple velocity components in a single beam and neither of them is well-resolved not complete = For the last cloud, No. 71 (no data)
History: From electronic version of the journal
(End) Patricia Vannier [CDS] 29-Jun-2006
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

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