Table 4.
Surface density of star formation for the sample galaxies with detected halos and the advection velocity of cosmic ray electrons produced in the disk.
| Name | ΣSFR | vadv |
|---|---|---|
| (M⊙ yr−1 kpc−2) | (km s−1) | |
| ESO 005-G004 | 0.0036 | 170 |
| ESO 079-G003 | 0.0096 | 253 |
| ESO 163-G011 | 0.01 | 257 |
| ESO 209-G009 | 0.0042 | 180 |
| IC 3908 | 0.0117 | 274 |
| NGC 1406 | 0.0086 | 241 |
| NGC 1421 | 0.0053 | 198 |
| NGC 1532 | 0.0020 | 132 |
| NGC 2221 | 0.0159 | 311 |
| NGC 4666 | 0.0095 | 252 |
| NGC 7090 | 0.0027 | 150 |
Notes. The surface density of star formation was obtained as ΣSFR = SFR/ASF, where the SFR are those listed in Table 1 and and ASF was obtained from the radio diameters listed in Table 2. The advection velocity of the cosmic rays was obtained using Eq. (15) (Heesen 2021).
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.