| vS | very small, < 30″ | |
| S | small, 30″ to 2′ or 3′ | |
| L | large, > 2′ or 3′ | |
| B | bright | |
| D | double | |
| E | elongated | |
| F | faint | |
| iF | irregular figure | |
| M | middle or in the middle | |
| N | nucleus | |
| R | round | |
| b | brighter | |
| bn | brighter toward the north side | |
| bs | brighter toward the south side | |
| bp | brighter toward the preceding side | |
| bf | brighter toward the following side | |
| bsw | brightest toward the south-west | |
| bM | brighter toward the middle | |
| dif | diffused | |
| diffic | difficult | |
| eF | extremely faint | |
| g | gradually | |
| i | irregular | |
| l | little | |
| m | much | |
| p | pretty | |
| pB | pretty bright | |
| pF | pretty faint | |
| sc | scattered | |
| stell | stellar | |
| sbM | suddenly brighter toward the middle | |
| v | very | |
| vbM | very much brighter toward the middle | |
| vS | very small | |
| F*inv | faint star involved | |
| ◯ | planetary |
Positions of Known Nebulæ Determined from the Crossley Negatives.