J/A+A/476/1243      Millimeter continuum mapping of Cygnus X      (Motte+, 2007)

The earliest phases of high-mass star formation: a 3 square degree millimeter continuum mapping of Cygnus X. Motte F., Bontemps S., Schilke P., Schneider N., Menten K.M., Broguiere D. <Astron. Astrophys. 476, 1243 (2007)> =2007A&A...476.1243M 2007A&A...476.1243M
ADC_Keywords: Molecular clouds ; Photometry, infrared ; Radio continuum Keywords: dust, extinction - HII regions - ISM: structure - stars: formation - submillimeter Description: We report on a millimeter continuum survey of the entire Cygnus X molecular complex. We used the MAMBO and MAMBO-2 bolometer arrays on the IRAM 30m telescope to map a 3deg2 area at 1.2mm (see fits files of Figures 2, kept to 11" resolution). Our MAMBO-2 imaging gives a complete view of the cloud structures ranging from 0.03pc to 5pc, i.e. from dense cores to clumps. We perform a multi-resolution analysis to extract 129 compact dense cores (∼0.1pc, see Table 1) and identify 40 massive large-scale clumps (∼0.7pc, see Table 2). The 21um fluxes arising from dense cores are taken from the MSX point source catalog (MSX C6, Cat. V/114). File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 166 129 Dense cores (compact cloud fragments) identified in Cygnus X refs.dat 66 13 References table2.dat 94 40 Clumps (large-scale cloud structures) identified in Cygnus X figs.dat 38 10 List of FITS files containing the 1.2mm observations fits/* . 10 FITS files of the images -------------------------------------------------------------------------------- See also: V/114 : MSX6C Infrared Point Source Catalog (Egan+ 2003) J/ApJS/74/181 : Small-diameter radiosources catalogue (Zoonematkermani+, 1990) J/A+A/241/551 : Radio continuum in Cygnus X region (Wendker+ 1991) J/ApJS/91/659 : Ultracompact HII regions radio images (Kurtz+ 1994) J/A+A/336/339 : VLA observations of ultracompact HII regions (Molinari+ 1998) J/A+A/375/539 : JHK photometry of compact HII regions in Cyg X (Comeron+, 2001) J/A+A/432/737 : General Catalogue of 6.7GHz Methanol Masers (Pestalozzi+, 2005) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 A5 --- --- [CygX-] 6- 9 A4 --- CygX Dense core number (Nnn, NWnn, or Snn) 11- 26 A16 --- Name Name (JHHMMSS.s+DDMMSS) 28- 31 I4 mJy Speak Peak flux at 1.2mm, in mJy/beam (1) 33- 36 F4.2 pc FWHMa Dense core FWHM size, major axis (1) 37 A1 --- --- [x] 38- 41 F4.2 pc FWHMb Dense core FWHM size, minor axis (1) 43- 47 I5 mJy Sint Integrated flux at 1.2mm (1) 49 A1 --- l_M(40K) Limit flag on M(40K) 50- 52 I3 solMass M(40K) ? Dense core mass with Tdust=40K (2) 54- 56 I3 solMass M(20K) Dense core mass with Tdust=20K (2) 58 A1 --- l_nH2(40K) Limit flag on nH240K 59- 64 E6.2 cm-3 nH2(40K) ? Volume-averaged H2 density, number with Tdust=40K (3) 66- 71 E6.2 cm-3 nH2(20K) Volume-averaged H2 density, number with Tdust=20K (3) 73- 79 F7.2 Jy S21um ?=- MSX flux at 21 microns (4) 80 A1 --- n_S21um [A] A: sources are seen in absorption at 8um 82 A1 --- n_CygX [*] Individual note (5) 84- 88 A5 --- ref(1) ? Reference for cm free-free, if exists, in refs.dat file (6) 90-109 A20 --- Maser Maser molecule, if exists (6) 111-115 A5 --- r_Maser Reference for Maser, in refs.dat file 117-166 A50 --- Note Names and comments -------------------------------------------------------------------------------- Note (1): Peak flux, deconvolved FWHM size, and integrated flux derived from a 2D-Gaussian fit to the 1.2mm map after background subtraction (cf. Sect. 3.2 and Appendix B). An upper limit FWHM of 0.03pc was assumed for unresolved fragments. Note (2): Mass derived from Col. 5 using Eq. (1) and assuming Kappa1.2mm=0.01cm2/g and Tdust=20K. A second estimate with Tdust=40K is made for HII regions and the brightest infrared protostars of Cygnus X. Note (3): Volume-averaged density derived from size and mass using Eq. (2). Note (4): The 21 microns fluxes are those given in the MSX point source catalog (MSX C6, Cat. V/114), except for CygX-N30, N43, N46, N47, N65 and S41, for which an aperture flux is measured on the MSX map. The MSX flux of two extended HII regions is equally distributed between CygX-N46 and N47, and between CygX-S18, S19, S20. All fragments detected at 21 microns are also detected at 8um with the exception of CygX-N30, N46, N47, and N65. "-" means that sources are undetected down to a flux of about 3Jy (completion level of the MSX 6C catalog in Cygnus X). Note (5): (*) observations of high-density tracers toward CygX-N4 suggest that this 1.2mm source does not correspond to a dense cloud fragment. Its nature is yet unclear but it is probably not a site for future or ongoing star formation. Note (6): Coincidence with stellar activity signatures -------------------------------------------------------------------------------- Byte-by-byte Description of file: refs.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I2 --- Ref Reference number 4- 22 A19 --- BibCode BibCode 24- 45 A22 --- Aut Author's name 47- 66 A20 --- Com Comments -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 A3 --- --- [Cl-] 4- 6 A3 --- Clump Clump number (Nnn, NWnn or Snn) 8- 23 A16 --- Name Name (JHHMMSS.s+DDMMSS) 25- 28 F4.2 pc FWHMa Clump FWHM size, major axis (1) 29 A1 --- --- [x] 30- 33 F4.2 pc FWHMb Clump FWHM size, minor axis (1) 35- 39 I5 mJy Sint Integrated flux at 1.2mm (1) 41- 44 I4 solMass Mass Clump mass (2) 46- 51 E6.2 cm-3 nH2 Volume-averaged density number (3) 53- 94 A42 --- Com Comments -------------------------------------------------------------------------------- Note (1): Deconvolved FWHM size and integrated flux derived from a 2D-Gaussian fit to the 1.2 mm map smoothed to a 55'' beam. Note (2): Mass derived from Col. 4 using Eq. (1) and assuming Kappa1.2mm=0.01cm2/g and Tdust=15K. Note (3): Volume-averaged density derived from size and mass, using Eq. (2). -------------------------------------------------------------------------------- Byte-by-byte Description of file: figs.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 A10 --- FITSfile Name of FITS file, in the "fits" subdirectory 12- 19 F8.4 deg RAdeg Image center, in decimal degrees (J2000) 21- 28 F8.4 deg DEdeg Image center, in decimal degrees (J2000) 30- 33 I4 pix Xdim Dimension (E-W) (1pix=4arcsec) 34 A1 --- --- [x] 35- 38 I4 pix Ydim Dimension (N-S) (1pix=4arcsec) -------------------------------------------------------------------------------- Acknowledgements: Frederique Motte, frederique.motte(at)cea.fr
(End) Frederique Motte [AIM/SAp], Patricia Vannier [CDS] 13-Sep-2007
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