A query to the Gaia Archive within 6 arc min of target name M51 finds 20 sources with phot_g_mean_mag <= 17.
Aladin Lite helps to locate them visually.
Five are circled in the lower half of the image in question:
Gaia source_id |
ra ° |
dec ° |
parallax (mas) |
magg |
1551894661845524736 |
202.4034 |
47.1522 |
8.854 ± 0.017 |
14.3 |
1551988532650838016 |
202.4205 |
47.1790 |
2.387 ± 0.041 |
16.4 |
1551988670089792256 |
202.4236 |
47.1979 |
0.632 ± 0.025 |
15.1 |
1551988425277200640 |
202.4323 |
47.1537 |
0.813 ± 0.025 |
15.2 |
1551988567010595840 |
202.4417 |
47.1800 |
1.536 ± 0.012 |
13.3 |
These parallaxes indicate distances between 113 and 1600 parsecs, well within the Milky Way.
Of the three sources circled in the upper half, two seem to be listed in Gaia EDR3 but do not have good parallaxes there.
Aladin Lite shows SIMBAD matches near all three in
Hwang and Lee 2008, a catalog of 2200 star clusters in M51.
HL2008 id |
ra ° |
dec ° |
magV |
Gaia source_id |
89770 |
202.494 |
47.216 |
20.0 |
1551988944968489984 |
13162 |
202.505 |
47.154 |
21.1 |
-- |
28066 |
202.531 |
47.167 |
19.8 |
1551987909882986368 |