J/A+A/628/A110      Photometry of submm cores in Vela C           (Massi+, 2019)

Dense cores and star formation in the giant molecular cloud Vela C. Massi F., Weiss, A., Elia D., Csengeri T., Schisano E., Giannini T., Hill T., Lorenzetti D., Menten K., Olmi L., Schuller F., Strafella F., de Luca M., Motte F., Wyrowski F. <Astron. Astrophys. 628, A110 (2019)> =2019A&A...628A.110M 2019A&A...628A.110M (SIMBAD/NED BibCode)
ADC_Keywords: Photometry, millimetric/submm ; Interstellar medium ; Molecular clouds Keywords: ISM: structure - submillimeter: ISM - ISM: individual objects: Vela Molecular Ridge - stars: formation - stars: protostars Abstract: We present the results of a study of the population of compact submm cores in Vela C, one of the molecular clouds making up the Vela Molecular Ridge, a nearby (∼700pc) star forming region in the Galactic plane. A large scale map of dust emission at 345GHz was obtained with LABOCA at the APEX telescope. Core retrieval and photometry were performed with the algorithms CuTEx and CLUMPFIND. Table 1 lists the sources retrieved by CuTEx. Table 2 lists the sources retrieved by CLUMPFIND. Description: Table 1 lists position, size (not deconvolved for beam size), position angle, peak flux density, integrated flux density, and error on the integrated flux density for the submm sources retrieved by CuTEx (Molinari at al., 2011A&A...530A.133M 2011A&A...530A.133M). The sources have been subdivided into starless cores associated with Vela C, protostellar cores associated with Vela C, and compact cores associated with the HII region RCW 34. CuTEx estimates source fluxes by fitting 2D Gaussian functions plus a plane to the sources, so isocontours are ellipses. For each source, the Full Widths at Half Maximum (FWHMs, in arcsec) along the two ellipse axis are given. The ellipse position angle (in degrees) is also given, measured counterclockwise from North to the first ellipse axis (labelled Ell1 in the table). Table 2 lists position, size (not deconvolved for beam size), peak flux density, integrated flux density, and error on the integrated flux density for the submm sources retrieved by CLUMPFIND (Williams at al., 1994ApJ...428..693W 1994ApJ...428..693W). The sources have been subdivided into compact cores associated with Vela C, compact cores associated with RCW 34, and compact cores with estimated size smaller than the beam size. Source size is given as the FWHM of the flux density spatial distribution along axis X and Y. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 63 564 Submm cores retrieved by CuTEx table2.dat 59 402 Submm cores retrieved by CLUMPFIND list.dat 85 1 Infirmatino on fits image fits/* . 1 Fits image -------------------------------------------------------------------------------- See also: J/A+A/399/147 : JHK photometry of C-cloud IRAS sources (Massi+, 2003) J/A+A/617/A63 : Star formation in the Vela Molecular Ridge (Prisinzano+, 2018) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- ID [1/564] Source identification code 5- 6 I2 h RAh Right ascension (J2000.0) 8- 9 I2 min RAm Right ascension (J2000.0) 11- 15 F5.2 s RAs Right ascension (J2000.0) 17 A1 --- DE- Declination sign (J2000.0) 18- 19 I2 deg DEd Declination (J2000.0) 21- 22 I2 arcmin DEm Declination (J2000.0) 24- 28 F5.2 arcsec DEs Declination (J2000.0) 30- 33 F4.1 arcsec Ell1 Ellipse axis 1 (FWHM) 35- 38 F4.1 arcsec Ell2 Ellipse axis 2 (FWHM) 40- 44 F5.1 deg PA Ellipse position angle 46- 50 F5.3 Jy/beam Flux Peak brightness at 345GHz 52- 56 F5.2 Jy IFlx Flux density at 345GHz 58- 61 F4.2 Jy e_IFlx ?=9.99 Flux density error (1) 63 A1 --- Flags [SPR] Flag (2) -------------------------------------------------------------------------------- Note (1): 9.99 means that the error could not be computed properly Note (2): Flags as follows: S = starless source P = protostellar source R = compact core associated with RCW 34 -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- ID [1/402] Source identification code 5- 6 I2 h RAh Right ascension (J2000.0) 8- 9 I2 min RAm Right ascension (J2000.0) 11- 15 F5.2 s RAs Right ascension (J2000.0) 17 A1 --- DE- Declination sign (J2000.0) 18- 19 I2 deg DEd Declination (J2000.0) 21- 22 I2 arcmin DEm Declination (J2000.0) 24- 28 F5.2 arcsec DEs Declination (J2000.0) 30- 34 F5.1 arcsec FWHMx Source size along axis X (FWHM) 36- 40 F5.1 arcsec FWHMy Source size along axis Y (FWHM) 42- 46 F5.3 Jy/beam Flux Peak brightness at 345GHz 48- 52 F5.2 Jy IFlx Flux density at 345GHz 54- 57 F4.2 Jy e_IFlx Flux density error 59 A1 --- Flags [CRU] Flags (1) -------------------------------------------------------------------------------- Note (1): Flags as follows: C = compact core associated with Vela C, R = compact core associated with RCW 34 U = compact core with size smaller than the APEX beam size -------------------------------------------------------------------------------- Byte-by-byte Description of file: list.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 F9.5 deg RAdeg Right Ascension of center (J2000) 10- 18 F9.5 deg DEdeg Declination of center (J2000) 20- 23 I4 --- Nx Number of pixels along X-axis 25- 28 I4 --- Ny Number of pixels along Y-axis 30- 34 I5 Kibyte size Size of FITS file 36- 65 A30 --- FileName Name of FITS file, in subdirectory fits 67- 85 A19 --- Title Title of the FITS file -------------------------------------------------------------------------------- Acknowledgements: Fabrizio Massi, fmassi(at)arcetri.astro.it References: Williams J., et al., 1994ApJ...428..693W 1994ApJ...428..693W Molinari S., et al., 2011A&A...530A.133M 2011A&A...530A.133M
(End) Fabrizio Massi [INAF-Arcetri, Italy], Patricia Vannier [CDS] 17-Jul-2019
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