Table 4
Spatial resolutions of the studied SNR-MC systems for a selection of relevant telescopes.
| Instrument | H.E.S.S. | Fermi/LAT | CTA | ALMA | ||
|
|
||||||
| Energy or λ | >100 GeV | 0.1 GeV | 100 GeV | 10 TeV | 72.5 mm | 362.5 μm |
| Ang. resolution | 0.1° | 3° | 0.04° | 1′ | 1′′ | 0.005′′ |
| Object | Linear spatial resolution for 90° inclination [pc] | |||||
|
|
||||||
| W49B | 14.0 | 419 | 5.6 | 2.3 | 0.0388 | 0.000194 |
| W44 | 5.8 | 173 | 2.3 | 1.0 | 0.0160 | 0.000080 |
| CTB 37A | 14.0 | 419 | 5.6 | 2.3 | 0.0388 | 0.000194 |
| 3C 391 | 12.6 | 377 | 5.0 | 2.1 | 0.0349 | 0.000175 |
Notes. The distances of the objects from Earth were taken from Table 2. The corresponding relative errors also apply to the spatial resolutions presented here. For ALMA, the maximum base length of 14.5 km was used. Sources for the instrumental data: H.E.S.S.: Aharonian et al. (2006), Fermi/LAT: http://www-glast.stanford.edu/instrument.html, CTA: http://www.cta-observatory.org/?q=node/26, ALMA: Peck & Beasley (2008).
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.