Table A.2
Derived properties of dense cores identified in HGBS maps of Orion B (template, full table only provided at the CDS).
| rNO | Core name | RA2000 | Dec2000 | Rcore | Mcore | Tdust |  |
 |
 |
 |
αBE | Core type | Comments |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| HGBS_J* | (h m s) | (° ′ ′′) | (pc) | (M⊙) | (K) | (1021 cm−2) | (1021 cm−2) | (104 cm−3) | (104 cm−3) | ||||
| (1) | (2) | (3) | (4) | (5) (6) | (7) ± (8) | (9) ± (10) | (11) | (12) (13) | (14) | (15) (16) | (17) | (18) | (19) |
| ⋯ | |||||||||||||
| 204 | 054126.7-014453 | 05:41:26.78 | –01:44:53.2 | 2.1e-02 3.9e-02 | 8.80 2.07 | 11.1 0.6 | 59.0 | 68.2 233.9 | 24.8 | 38.2 242.5 | 0.0 | 2 | |
| ⋯ | |||||||||||||
| 428 | 054202.9-020745 | 05:42:02.93 | –02:07:45.2 | 1.8e-02 3.7e-02 | 6.17 1.17 | 11.5 0.5 | 56.9 | 54.4 235.6 | 24.3 | 32.5 292.7 | 0.1 | 3 | |
| ⋯ | |||||||||||||
| 682 | 054316.0-025859 | 05:43:16.09 | –02:58:59.0 | 2.9e-02 4.6e-02 | 0.05 0.02 | 15.7 1.7 | 0.2 | 0.3 0.7 | 0.1 | 0.1 0.5 | 11.4 | 1 | |
| ⋯ |
Notes. Table entries are as follows: (1) core running number; (2) core name = HGBS_J prefix directly followed by a tag created from the J2000 sexagesimal coordinates; (3) and (4): right ascension and declination of core center; (5) and (6): geometrical average between the major and minor FWHM sizes of the core (in pc), as measured in the high-resolution column density map after deconvolution from the 18.2′′ HPBW resolution of the map and before deconvolution, respectively. (NB: both values provide estimates of the object’s outer radius when the core canbe approximately described by a Gaussian distribution, as is the case for a critical Bonnor-Ebert spheroid); (7) estimated core mass (M⊙) assuming the dust opacity law advocated by Roy et al. (2014); (9) SED dust temperature (K); (8) and (10) statistical errors on the mass and temperature, respectively, including calibration uncertainties, but excluding dust opacity uncertainties; (11) peak H2 column density, at the resolution of the 500 μm data, derived from a graybody SED fit to the core peak flux densities measured in a common 36.3′′ beam at all wavelengths; (12) average column density, calculated as 
, where Mcore is the estimated core mass (col. 7), Rcore the estimated core radius prior to deconvolution (col. 6), and μ = 2.8; (13) average column density calculated in the same way as for col. 12 but using the deconvolved core radius (col. 5); (14) beam-averaged peak volume density at the resolution of the 500 μm data, derived from the peak column density (col. 11) assuming a Gaussian spherical distribution:
; (15) average volume density, calculated as 
, using the estimated core radius prior to deconvolution; (16) average volume density, calculated in the same way as for col. 15 but using the deconvolved core radius (col. 5); (17) bonnor-Ebert mass ratio:
αBE = MBE,crit∕Mobs
(see text for details); (18) core type: 1-starless, 2-prestellar, 3-protostellar, or 0-tentative core. The latter is a likely extragalactic source (see comments); (19) comments: “no SED fit”, “tentative bound”, “N region”.
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