Table 3
Characteristics of starless sources extracted with Gaussclumps in the 870 μm continuum sum map of Cha III at scale 5.
Name | Ngcla | FWHMb | Rab | Npeakc | AVd | Mpeake | Mtote | M50″e | CMf | αBEg | npeakh | nmeanh | n50″h | cni |
(1000 AU)2 | (1021 cm-2) | (mag) | (M⊙) | (M⊙) | (M⊙) | (%) | (105 cm-3) | (104 cm-3) | (104 cm-3) | |||||
(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) | (12) | (13) | (14) | (15) |
|
||||||||||||||
Cha3-C1 | 1 | 17.1 × 8.8 | 2.0 | 16 | 5.0 | 0.097 | 1.55 | 0.29 | 33( 2) | 1.12 | 8.6 | 3.0 | 19.7 | 4.4(0.3) |
Cha3-C2 | 2 | 10.3 × 8.0 | 1.3 | 10 | 8 | 0.061 | 0.57 | 0.23 | 27( 3) | 0.55 | 5.5 | 2.7 | 15.5 | 3.5(0.4) |
Cha3-C3 | 3 | 7.8 × 3.3 | 2.4 | 8.8 | 4.2 | 0.053 | 0.20 | 0.11 | 47( 7) | 0.35 | 4.7 | 5.6 | 7.6 | 6.2(0.9) |
Cha3-C4 | 4 | 11.2 × 6.6 | 1.7 | 8.6 | 3.7 | 0.052 | 0.44 | 0.15 | 35( 5) | 0.45 | 4.6 | 2.5 | 10.1 | 4.6(0.6) |
Cha3-C5 | 5 | 9.6 × 6.9 | 1.4 | 8.1 | 5.7 | 0.049 | 0.37 | 0.13 | 37( 5) | 0.40 | 4.3 | 2.5 | 9.0 | 4.9(0.7) |
Cha3-C6 | 6 | 7.7 × 6.9 | 1.1 | 7.8 | 1.9 | 0.047 | 0.30 | 0.13 | 37( 6) | 0.36 | 4.2 | 2.7 | 8.7 | 4.8(0.7) |
Cha3-C7 | 7 | 8.3 × 4.7 | 1.8 | 7.6 | 5.1 | 0.046 | 0.23 | 0.10 | 44( 7) | 0.32 | 4.1 | 3.4 | 7.1 | 5.8(0.9) |
Cha3-C8 | 8 | 14.1 × 5.0 | 2.8 | 7.4 | 4.5 | 0.045 | 0.38 | 0.11 | 39( 6) | 0.40 | 4.0 | 2.3 | 7.7 | 5.2(0.8) |
Cha3-C9 | 9 | 12.5 × 4.6 | 2.7 | 7.4 | 4.9 | 0.045 | 0.32 | 0.11 | 41( 7) | 0.37 | 4.0 | 2.6 | 7.3 | 5.4(0.9) |
Cha3-C10 | 10 | 8.4 × 2.6 | 3.2 | 7.2 | 6 | 0.044 | 0.16 | 0.083 | 52(10) | 0.30 | 3.9 | 5.6 | 5.7 | 6.9(1.3) |
Cha3-C11 | 11 | 7.9 × 4.7 | 1.7 | 7.0 | 4.9 | 0.042 | 0.20 | 0.10 | 42( 7) | 0.29 | 3.7 | 3.2 | 6.8 | 5.5(1.0) |
Cha3-C12 | 12 | 11.2 × 5.9 | 1.9 | 6.7 | 7 | 0.040 | 0.31 | 0.10 | 40( 7) | 0.34 | 3.6 | 2.1 | 6.8 | 5.3(1.0) |
Cha3-C13 | 13 | 9.3 × 4.6 | 2.0 | 6.8 | 4.6 | 0.041 | 0.22 | 0.10 | 41( 7) | 0.30 | 3.6 | 2.8 | 6.8 | 5.4(1.0) |
Cha3-C14 | 14 | 10.4 × 2.4 | 4.3 | 6.6 | 8 | 0.040 | 0.17 | 0.083 | 48( 9) | 0.30 | 3.5 | 4.8 | 5.6 | 6.3(1.2) |
Cha3-C15 | 15 | 8.9 × 5.0 | 1.8 | 6.4 | 5.3 | 0.039 | 0.21 | 0.088 | 44( 9) | 0.28 | 3.5 | 2.6 | 6.0 | 5.8(1.1) |
Cha3-C16 | 16 | 9.6 × 4.5 | 2.1 | 6.0 | 5.4 | 0.037 | 0.20 | 0.082 | 44( 9) | 0.27 | 3.2 | 2.5 | 5.6 | 5.8(1.2) |
Cha3-C17 | 17 | 3.3 × 2.1 | 1.6 | 6.1 | 5.7 | 0.037 | 0.053 | 0.048 | 77(21) | 0.18 | 3.3 | 10.7 | 3.3 | 10.0(2.7) |
Cha3-C18 | 18 | 4.3 × 3.3 | 1.3 | 6.2 | 9 | 0.038 | 0.091 | 0.12 | 30( 5) | 0.21 | 3.4 | 6.1 | 8.4 | 4.0(0.7) |
Cha3-C19 | 19 | 6.8 × 3.5 | 1.9 | 6.0 | 4.8 | 0.036 | 0.13 | 0.091 | 40( 8) | 0.23 | 3.2 | 3.9 | 6.2 | 5.2(1.1) |
Cha3-C20 | 20 | 4.8 × 3.8 | 1.2 | 6.1 | 9 | 0.037 | 0.10 | 0.083 | 45( 9) | 0.22 | 3.3 | 4.8 | 5.6 | 5.9(1.2) |
Cha3-C21 | 21 | 9.5 × 2.1 | 4.5 | 5.5 | 5.9 | 0.033 | 0.11 | 0.060 | 55(14) | 0.22 | 3.0 | 4.5 | 4.0 | 7.3(1.8) |
Cha3-C22 | 22 | 5.8 × 3.8 | 1.5 | 5.7 | 4.3 | 0.034 | 0.11 | 0.073 | 47(10) | 0.21 | 3.0 | 3.8 | 5.0 | 6.1(1.4) |
Cha3-C23 | 23 | 17.7 × 3.1 | 5.8 | 5.6 | 2.8 | 0.034 | 0.26 | 0.069 | 49(11) | 0.32 | 3.0 | 2.4 | 4.7 | 6.4(1.5) |
Cha3-C24 | 24 | 9.6 × 6.0 | 1.6 | 5.5 | 7 | 0.033 | 0.23 | 0.091 | 37( 8) | 0.27 | 3.0 | 1.8 | 6.2 | 4.8(1.0) |
Cha3-C25 | 25 | 7.2 × 2.1 | 3.4 | 5.4 | 4.3 | 0.032 | 0.081 | 0.052 | 62(17) | 0.18 | 2.9 | 4.9 | 3.5 | 8.1(2.2) |
Cha3-C26 | 26 | 2.3 × 2.1 | 1.1 | 5.2 | 3.7 | 0.031 | 0.039 | 0.054 | 58(16) | 0.16 | 2.8 | 12.9 | 3.6 | 7.6(2.1) |
Cha3-C27 | 27 | 6.7 × 2.1 | 3.2 | 5.1 | 2.3 | 0.031 | 0.071 | 0.049 | 63(18) | 0.17 | 2.7 | 4.9 | 3.3 | 8.2(2.4) |
Cha3-C28 | 28 | 4.9 × 2.1 | 2.3 | 5.1 | 3.2 | 0.031 | 0.056 | 0.038 | 81(27) | 0.16 | 2.7 | 6.2 | 2.6 | 10.7(3.6) |
Cha3-C29 | 29 | 5.3 × 3.0 | 1.7 | 5.1 | 3.7 | 0.031 | 0.082 | 0.061 | 50(13) | 0.18 | 2.7 | 4.6 | 4.2 | 6.5(1.7) |
Notes.
Numbering of Gaussclumps sources like in Table 2.
Deconvolved physical source size (FWHM) and aspect ratio (Ra) of the fitted Gaussian. The minimum size that can be measured is 2100 AU (see Sect. 4.3.2). The aspect ratio is the ratio of the deconvolved sizes along the major and minor axes.
Mass in the central beam (HPBW = 21.2″) (Mpeak), total mass derived from the Gaussian fit (Mtot), and mass computed from the flux measured in an aperture of 50″ in diameter (M50″). The statistical rms uncertainties of Mpeak and M50″ are 0.006 and 0.010 M⊙, respectively.
Ratio Mtot/MBE, with MBE the critical Bonnor-Ebert mass (see Sect. 4.3.6).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.