Table 4
Observed and deconvolved source sizes (arcsec).
Source (a) | Major axis | Minor axis | Position angle (degrees) | Deconvolved (b) | Model (c) | 850–870 μm (d) |
---|---|---|---|---|---|---|
IRAS 05358 | 12.0 (0.5) | 9.3 (0.4) | −46 (6) | 4.4 | 15.0 | 30.0 |
IRAS 16272 | 15.9 (0.7) | 11.8 (0.6) | −34 (5) | 8.8 | 18.0 | 50.0 |
NGC 6334 I(N) | 17.2 (0.5) | 12.5 (0.4) | 38 (3) | 11.3 | 21.6 | 42.0 |
W43 MM1 | 15.8 (1.6) | 12.8 (1.2) | −89 (15) | 15.5 | 11.8 | 27.0 |
DR21(OH) | 12.4 (0.4) | 11.1 (0.4) | −8 (11) | 5.4 | 28.8 | 33.0 |
W3 IRS5 | 14.1 (0.3) | 12.0 (0.3) | −9 (5) | 7.8 | 40.0 | 57.0 |
IRAS 18089 | 11.0 (0.9) | 9.5 (0.8) | −37 (21) | -0- | ... | 17.0 |
W33A | 11.6 (0.7) | 10.0 (0.6) | −44 (16) | 5.1 | ... | 30.0 |
AFGL 2591 | 11.3 (0.6) | 9.7 (0.5) | 76 (12) | 3.8 | 25.2 | 25.2 |
G327-0.6 | 14.3 (0.5) | 10.2 (0.4) | 67 (4) | 5.5 | ... | 24.0 |
NGC 6334I | 16.1 (0.5) | 15.0 (0.4) | 88 (13) | 12.6 | ... | 40.0 |
G29.96 | 10.7 (0.3) | 9.6 (0.3) | −13 (11) | 3.0 | ... | 16.0 |
G31.41 | 9.9 (0.9) | 7.5 (0.7) | −5 (13) | -0- | ... | 15.0 |
G5.89 | 10.9 (0.2) | 10.0 (0.2) | −29 (7) | 3.9 | ... | 28.0 |
G10.47 | 11.9 (0.7) | 10.2 (0.6) | −47 (14) | 5.5 | ... | 10.0 |
G34.26 | 22.4 (1.0) | 16.9 (0.8) | −17 (4) | 16.9 | ... | 25.0 |
W51N-e1 | 14.5 (0.7) | 10.9 (0.5) | −63 (6) | 8.2 | ... | 27.0 |
Notes. (a) The source fitting failed for IRAS 18151 and NGC 7538. (b)Equivalent circular axis; a value of zero means that the source is unresolved. (c) From Chavarría et al. (2010) for W3 IRS5, Herpin (priv. comm.) for AFGL 2591; other sources from Herpin et al. (2016). (d) 3σ radii from Van der Tak et al. (2013).
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.