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J/ApJS/196/18     CO survey of galactic molecular clouds. II.   (Bieging+, 2011)

The Arizona radio observatory CO mapping survey of galactic molecular clouds. II. The W3 region in CO J = 2-1, 13CO J = 2-1, and CO J = 3-2 emission. Bieging J.H., Peters W.L. <Astrophys. J. Suppl. Ser., 196, 18 (2011)> =2011ApJS..196...18B
ADC_Keywords: Molecular clouds ; Radio lines ; H II regions ; Interstellar medium ; Millimetric/submm sources Keywords: H II regions - ISM: clouds - ISM: individual objects (W3) - ISM: kinematics and dynamics - ISM: molecules Abstract: We present fully sampled 38" resolution maps of the CO and 13CO J=2-1 lines in the molecular clouds toward the HII region complex W3. The maps cover a 2.0°x1.67° section of the galactic plane and span -70 to -20km/s (LSR) in velocity with a resolution of ∼1.3km/s. The velocity range of the images includes all the gas in the Perseus spiral arm. We also present maps of CO J=3-2 emission for a 0.5°x0.33° area containing the HII regions W3 Main and W3(OH). The J=3-2 maps have velocity resolution of 0.87km/s and 24" angular resolution. Color figures display the peak line brightness temperature, the velocity-integrated intensity, and velocity channel maps for all three lines, and also the (CO/13CO) J=2-1 line intensity ratios as a function of velocity. The line intensity image cubes are made available in standard FITS format as electronically readable files. We compare our molecular line maps with the 1.1mm continuum image from the BOLOCAM Galactic Plane Survey (BGPS). From our 13CO image cube, we derive kinematic information for the 65 BGPS sources in the mapped field, in the form of Gaussian component fits. Description: Observations were made with the Heinrich Hertz Submillimeter Telescope (HHT) on Mt. Graham, AZ; in several observing sessions from 2005 June to 2008 April. The J=2-1 lines of the CO isotopologues 12C16O (hereafter CO) and 13C16O (hereafter 13CO) were mapped over a 2.00°x1.67° field covering the galactic coordinate ranges l=132.5° to 134.5°, b=0° to +1.67°. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table2.dat 53 77 The 13CO (J=2-1) line properties at BGPS (BOLOCAM Galactic Plane Survey) source positions
See also: J/ApJS/188/123 : The Bolocam Galactic Plane Survey. II. (Rosolowsky+, 2010) J/ApJS/191/232 : CO survey of W51 molecular cloud (Bieging+, 2010) J/ApJ/654/338 : Spitzer photometry in W3 molecular cloud (Ruch+, 2007) J/MNRAS/379/663 : 850um observations of W3 giant molecular cloud (Moore+, 2007) J/A+AS/124/205 : W3 star-forming region 345 GHz survey (Helmich+ 1997) Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1- 4 I4 --- BGPS BGPS catalog number; Rosolowsky et al. 2010, Cat. J/ApJS/188/123 6- 12 F7.3 deg GLON Galactic longitude of BGPS peak 14- 18 F5.3 deg GLAT Galactic latitude of BGPS peak 20- 24 F5.3 Jy F1.1 BGPS 1.1mm continuum flux density (1) 26- 30 F5.1 K.km/s 13CO Integrated intensity of ^13^CO (J=2-1) emission line (2) 32 I1 --- m_BGPS The ^13^CO line Gaussian fit component number (3) 34- 38 F5.2 K Amp Main-beam brightness temperature amplitude (4) 40- 44 F5.1 km/s Vpeak LSR velocity of peak (4) 46- 48 F3.1 km/s FWHM Velocity full-width at half-maximum (4) 50- 53 F4.2 K FRMS RMS of residual to Gaussian fit (5)
Note (1): Within 40 arcsec diameter aperture. Fluxes have not been scaled by any correction factor (cf. Rosolowsky et al. 2010, Cat. J/ApJS/188/123). Note (2): In main-beam brightness temperature. Note (3): For multiple component fits. Note (4): Of 13CO line Gaussian fit component. Note (5): Including all components, in main-beam brightness temperature.
Nomenclature note: BGPS objects are <BGPS GLLL.lll+BB.bbb> in Simbad. History: From electronic version of the journal References: Bieging et al. Paper I. (W51) 2010ApJS..191..232B Cat. J/ApJS/191/232 Burleigh et al. Paper III. (Serpens) 2013ApJS..209...39B Cat. J/ApJS/209/39 Bieging et al. Paper IV. (NGC 1333) 2014ApJS..214....7B Cat. J/ApJS/214/7
(End) Greg Schwarz [AAS], Emmanuelle Perret [CDS] 16-Nov-2011
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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