| ID | Type of source
|
Morphological type
|
Number of |
| (ADFS) | counterparts
|
||
| 1 | Galaxy/IRS/RS | Sb | 1 |
| 2 | Galaxy in Pair of Interacting Galaxies/IRS/RS | E | 1 |
| 3 | Galaxy/IRS/RS/other | Sa | 1 |
| 4 | Stardust Galaxy IR emission line up with | S0, SA0- pec: HII BCDG | 1 |
| Super Star Cluster/IRS/RS/other | |||
| 5 | Galaxy/IRS/RS | S | 2 |
| 6 | Galaxy/IRS | - | 4 |
| 7 | Galaxy in Cluster of Galaxies/IRS | S01 | 1 |
| 8 | Galaxy in Cluster of Galaxies/IRS | Sb1 | 2 |
| 9 | Galaxy in Cluster of Galaxies | Sb1 | 3 |
| 10 | Galaxy in Cluster of Galaxies/IRS/RS | S00 pec1 | 1 |
| 11 | Galaxy in Cluster of Galaxies/IRS/RS | SB1 | 1 |
| 12 | IRS | - | 1 |
| 13 | Galaxy/IRS | - | 2 |
| 14 | Galaxy/IRS/RS | - | 2 |
| 15 | Galaxy/IRS | - | 3 |
| 16 | IRS/Galaxy in Pair of Galaxies | - | 2 |
| 17 | Interacting Galaxies/IR/RS | Sbc pec | 3 |
| 18 | Galaxy/IRS | S | 1 |
| 19 | Galaxy/IRS | - | 2 |
| 20 | Galaxy/IRS | - | 1 |
| 21 | Galaxy/IRS | SAB | 1 |
| 22 | Galaxy/IRS | S | 2 |
| 23 | Interacting Galaxies | cG (compact G), Chain of 3 galaxies | 1 |
| 24 | Galaxy/IRS | S | 2 |
| 26 | Galaxy | - | 2 |
| 27 | IRS | - | 1 |
| 29 | Galaxy/IRS | S0a | 1 |
| 30 | IRS/Galaxy | - | 1 |
| 31 | IRS/Galaxy | - | 1 |
| 39 | Galaxy/IRS | S0 | 3 |
| 41 | Galaxy/IRS | - | 2 |
| 42 | Galaxy/IRS | - | 1 |
| 43 | IRS/Galaxy | - | 1 |
| 45 | Galaxy in Cluster of Galaxies/IRS | Sbp1 | 1 |
| 46 | Galaxy/IRS | - | 1 |
| 48 | Galaxy/IRS | - | 1 |
| 49 | Galaxy | - | 2 |
| 50 | Galaxy/IRS | S | 1 |
| 51 | Galaxy/IRS/RS | SB | 1 |
| 52 | IRS/Galaxy | - | 1 |
| 56 | Galaxy/IRS | - | 5 |
| 64 | Galaxy/IRS | Sc | 1 |
| 65 | Galaxy in Cluster of Galaxies/IRS | S01 | 1 |
| 69 | Galaxy/ IRS | - | 2 |
| 72 | Galaxy in Cluster of Galaxies/IRS | Sbb pec1 | 2 |
| 73 | IRS | - | 1 |
| 82 | Galaxy | - | 1 |
| 103 | Galaxy in Cluster of Galaxies/IRS | Sb1 | 2 |
Notes. (a) The object classification: Galaxy means that it has been identified as a galaxy, IRS means that it has been previously identified as the infra-red source, RS means that it has been identified as the radio source, ``other'' means that it has been observed in some other (UV or X-ray) wavelengths. This column contains also the available information about the object's environment - whether it is an object from the cluster of galaxies (in this case it always applies to Abell S0463) or an interacting group of galaxies. (b) The object's indicative morphological type, as provided by the NED. (c) The number of counterparts found for each object in our 40'' search range, which may be treated as a very crude indicator of the local environment of an investigated object. (1) Dressler (1980a).
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.