J/ApJ/653/383    SCUBA observations in Orion A South region   (Johnstone+, 2006)

Large-area mapping at 850µm. V. Analysis of the clump distribution in the Orion A South molecular cloud. Johnstone D., Bally J. <Astrophys. J., 653, 383-397 (2006)> =2006ApJ...653..383J 2006ApJ...653..383J
ADC_Keywords: Molecular clouds ; Millimetric/submm sources Keywords: infrared: ISM: continuum - ISM: individual (HH 1/2, HH 34, L1641N, OMC 4, OMC 5, Orion A South) - ISM: structure - stars: formation Abstract: We present results from a 2300arcmin2 survey of the Orion A molecular cloud at 450 and 850um using the Submillimeter Common-User Bolometer Array (SCUBA) on the James Clerk Maxwell Telescope. The region mapped lies directly south of the OMC 1 cloud core and includes OMC 4, OMC 5, HH 1/2, HH 34, and L1641N. We identify 71 independent clumps in the 850um map and compute size, flux, and degree of central concentration in each. Description: The data covering the Orion A South region were obtained between 1997 and 2002 using SCUBA at the James Clerk Maxwell Telescope (JCMT). File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 74 71 Clump properties in Orion A south derived from 850um data -------------------------------------------------------------------------------- See also: J/ApJ/559/307 : Sub-mm mapping in Ori B molecular cloud (Johnstone+, 2001) J/ApJ/639/259 : Sub-mm clumps in Ori B South molecular cloud (Johnstone+, 2006) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 12 A12 -- SMMJ Name formed with J2000.0 positions (HHMMmm+DDMMm), [JB2006] SMM JHHMMmm+DDMMm in Simbad 14- 15 I2 --- [JB2006] Sequential number 17- 18 I2 h RAh Right ascension (J2000.0) (1) 20- 21 I2 min RAm Right ascension (J2000.0) (1) 23- 26 F4.1 s RAs Right ascension (J2000.0) (1) 28 A1 --- DE- Declination sign (J2000.0) (1) 29- 30 I2 deg DEd Declination (J2000.0) (1) 32- 33 I2 arcmin DEm Declination (J2000.0) (1) 35- 36 I2 arcsec DEs Declination (J2000.0) (1) 38- 42 F5.2 Jy S850 Total flux at 850um (2) 44- 47 F4.2 Jy Sp850 Peak flux at 850um (Jy/beam) (2) 49- 50 I2 10+3AU Reff Effective radius (2) 52- 55 F4.2 --- C Concentration parameter (3) 57- 58 I2 K Td Dust temperature (3) 60- 62 F3.1 [K/cm3] log(P/k) External pressure (3) 64- 68 F5.2 solMass M Mass at dust temperature (3) 70- 74 F5.2 solMass M20K Mass at dust temperature Td=20K (4) -------------------------------------------------------------------------------- Note (1): Position of peak surface brightness within clump (accurate to 3"). Note (2): Radius, peak flux, and total flux are derived from CLFIND (Williams et al., 1994, Cat. J/ApJ/428/693). The peak flux and total flux have uncertainties of about 20%, mostly due to absolute flux calibration. The radius has not been deconvolved from the telescope beam. Note (3): Quantities derived from Bonnor-Ebert analysis (see text). Note (4): Mass derived from the total flux assuming Td=20K and k850=0.02cm2/g. -------------------------------------------------------------------------------- History: From electronic version of the journal References: Johnstone et al., Paper I 2000ApJS..131..505J 2000ApJS..131..505J Johnstone et al., Paper II 2000ApJ...545..327J 2000ApJ...545..327J Johnstone et al., Paper III 2001ApJ...559..307J 2001ApJ...559..307J, Cat. J/ApJ/559/307 Johnstone et al., Paper IV 2006ApJ...639..259J 2006ApJ...639..259J, Cat. J/ApJ/639/259
(End) Patricia Vannier [CDS] 31-Jul-2008
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