Index Catalog Objects: IC 5200 (original) (raw)

QuickLinks:
5200, 5201, 5202, 5203, 5204, 5205, 5206, 5207, 5208, 5209, 5210, 5211, 5212, 5213, 5214, 5215, 5216,
5217, 5218, 5219, 5220, 5221, 5222, 5223, 5224, 5225, 5226, 5227, 5228, 5229, 5230, 5231, 5232, 5233,
5234, 5235, 5236, 5237, 5238, 5239, 5240, 5241, 5242, 5243, 5244, 5245, 5246, 5247, 5248, 5249

Page last updated Jul 3, 2024
Updated IC 5204
WORKING 5200: Precess Dreyer positions, check IDs, add pix
WORKING: Check for HLA images

IC 5200 (= PGC 68660)
Discovered (Aug 21, 1900) by DeLisle Stewart
A magnitude 15.3 spiral galaxy (type SA(r)c?) in Tucana (RA 22 22 15.2, Dec -65 45 58)

Historical Identification: Per Dreyer, IC 5200 (DeLisle Stewart #747, 1860 RA 22 12 02, NPD 156 27) is "most extremely faint, extremely small, round, faint star 1 arcmin to northwest".
Physical Information: Apparent size 0.7 by 0.4 arcmin. Distance (and therefore actual size) unknown.

DSS image of region near spiral galaxy IC 5200
Above, a 12 arcmin wide DSS image centered on IC 5200
Below, a 0.9 arcmin wide DSS image of the galaxy
DSS image of spiral galaxy IC 5200

IC 5201 (= PGC 68618)
Discovered (1900) by Joseph Lunt
A magnitude 10.8 spiral galaxy (type SB(rs)cd?) in Grus (RA 22 20 57.4, Dec -46 02 09)

Historical Identification: Per Dreyer, IC 5201 (Lunt (#4), 1860 RA 22 12 44, NPD 136 46.0) has "no description". The position precesses to RA 22 21 19.7, Dec -46 03 52, about 4.2 arcmin southeast of the nucleus of the galaxy listed above, but there is nothing else nearby and the galaxy is far larger than the distance between it and Lunt's position, so the identification is certain.
Physical Information: Based on a recessional velocity of 915 km/sec (and H0 = 70 km/sec/Mpc), IC 5201 is about 40 to 45 million light years away, further than redshift-independent distance estimates of 13 to 35 million light years, but the same as the "over 40 million" light year distance quoted in the press release for the HST image below. Given that and its apparent size of about 9.0 by 3.8 arcmin (from the images below), it is about 110 to 115 thousand light years across. Since the galaxy is relatively close, the HST image can show individual stars in the galaxy, as well as clusters of stars and star-forming regions.

DSS image of region near spiral galaxy IC 5201
Above, a 12 arcmin wide DSS image centered on IC 5201
Below, a 6.75 by 8.75 arcmin wide image of the galaxy
(Image Credit & © Carnegie-Irvine Galaxy Survey; used by permission)
Carnegie-Irvine Galaxy Survey image of spiral galaxy IC 5201
Below, a 2.75 by 3.5 arcmin wide HST image of the nucleus of the galaxy (Image Credit ESA/Hubble & NASA)
HST image of the nucleus of spiral galaxy IC 5201
Below, a 6.75 by 8.75 arcmin wide image of the galaxy showing the position of the HST image
(Image Credits as for previous two images)
HST image of part of spiral galaxy IC 5201 overlaid on the Carnegie-Irvine Galaxy Survey image of the whole galaxy

IC 5202 (= PGC 68707)
Discovered (Aug 21, 1900) by DeLisle Stewart
A magnitude 13.8 spiral galaxy (type SBc??) in Tucana (RA 22 22 55.3, Dec -65 48 09)

Historical Identification: Per Dreyer, IC 5202 (DeLisle Stewart #748, 1860 RA 22 12 44, NPD 156 30) is "a remarkable object, extremely faint, very small, stellar nucleus, spiral".
Physical Information: Apparent size 1.3 by 0.6? arcmin.

IC 5203 (= PGC 68684)
Discovered (Jul 16, 1904) by Royal Frost
A magnitude 14.2 spiral galaxy (type SBc??) in Tucana (RA 22 22 34.3, Dec -59 46 24)

Historical Identification: Per Dreyer, IC 5203 (Frost #1226, 1860 RA 22 13 04, NPD 150 29) has a "brighter middle, magnitude 15".
Physical Information: Apparent size 1.3 by 0.7? arcmin.

WORKING HERE: need to clean-up PanSTARRS image
IC 5204 (perhaps (??) = NGC 7298, or NGC 7300 (and if = NGC 7300, also = PGC 69040 = PGC 930291 = MCG -02-57-011)
Recorded (Aug 8, 1896) by Lewis Swift (and later listed as IC 5204)
Either a lost or nonexistent object in Aquarius (RA 22 20 41.7, Dec -14 23 59)
or if = NGC 7300, a magnitude 12.9 spiral galaxy (type SB(s)b?) in Aquarius (RA 22 30 59.9, Dec -14 00 13)

Historical Identification: Per Dreyer, IC 5204 (Lewis Swift list XI (#212), 1860 RA 22 13 10, NPD 105 06.1) is "very faint, very much extended." The position precesses to RA 22 20 41.7, Dec -14 23 59 (whence the position shown above), but there is nothing there nor near there, so the most reasonable conclusion is that IC 5204 is "lost or nonexistent".
Argument In Favor of Duplicate Observation of NGC 7300: Per Corwin, Swift found this on the same night that he found IC 5228 (= NGC 7302), and describes it as "very faint, extremely extended, a ray; preceding (western) of 2," the other presumably being IC 5228, since his description for that reads "pretty bright, pretty small, round; bright star near to south; following (eastern) of 2," which would suggest that IC 5204 is the western member of the supposed pair. There is no doubt that IC 5228 = NGC 7302, because the positions match to within 10 seconds of time, and there is nothing else nearby that could be Swift's object. The bright star is there, and NGC 7302 is a "following of 2" with the preceding object possibly being NGC 7300, which means that IC 5204 could be a duplicate entry for NGC 7300.
The problem is that Swift's position for IC 5204 is 10 minutes west and 20 arcmin south of NGC 7300, which would be an extremely poor position, even for Swift. Corwin's suggestion is that Swift made "simple digit errors" in his position, and that his "nova" was simply the bright inner part of NGC 7300. Gottlieb agrees with Corwin's argument and simple digit errors aren't rare, so although IC 5204 could be a lost or nonexistent object, it might be a duplicate entry for NGC 7300. But "might" is not the same as "certainly", so I have added a question mark to that suggestion.
(Weak) Argument In Favor of Duplicate Observation of NGC 7298: Thinking in terms of "simple digit errors", the most common is a change of 1 unit, and we could apply such a change to the 10's values in both of Swift's positions (Corwin points out that both the RA and Dec would have to be changed to fit NGC 7300, by 10 minutes for the RA, and 20 for the Dec). Perhaps instead of having different "simple digit errors" in each position, we should alter both values by only 1 unit. In that case Swift's position for IC 5204 (1900 RA 22 25 19, Dec -14 54.1) would become RA 22 15 19, Dec -14 44.1, which precesses to (2000) RA 22 30 39.9, Dec -14 13 21, which lies only 2.8 arcmin west-southwest of NGC 7298, lies only 4 arcmin south of IC 5228 (which would fit the concept of sweeping along a parallel of declination by letting the sky move past the telescope's target just as well as for NGC 7300), and is fainter than IC 5228, which fits Swift's description of being fainter than NGC 7302, but does not fit his description of IC 5204 being extremely extended. So although the wide-field image below shows NGC 7298 as well as NGC 7300 and 7302, and there is an extremely remote possibility that IC 5204 is NGC 7298, although in an earlier version of this entry I attached (= IC 5204?) to the image of NGC 7298, I have decided to remove that suggestion.
Conclusion: Given the fact that in the NGC Swift lists two galaxies in the region, and there are two galaxies in the region that fit his description (though not his positions), it is hard to believe that he actually only saw one. So although it is possible that IC 5204 is "lost or nonexistent", as shown above, odds are that it is NGC 7300, as also shown, albeit with a question mark.
Physical Information: If IC 5204 is lost or nonexistent, there is nothing to say; but if, as seems possible (albeit unlikely), it is NGC 7300, then see that for anything more.

DSS image of region near the NGC position for the 'lost or nonexistent' IC 5204
Above, a 12 arcmin wide DSS image centered on the NGC position for the "lost or nonexistent" IC 5204
Below, a 25 by 22 arcmin wide PanSTARRS image centered between NGC 7298, NGC 7300 and NGC 7302
PanSTARRS image centered between NGC 7300, which may be IC 5204, and NGC 7298, which is not likely to be IC 5204

IC 5205 (= PGC 68700)
Discovered (Jul 16, 1904) by Royal Frost
A magnitude 15.2 spiral galaxy (type Sc??) in Tucana (RA 22 22 47.7, Dec -59 47 12)

Historical Identification: Per Dreyer, IC 5205 (Frost #1227, 1860 RA 22 13 16, NPD 150 30) has a "brighter middle, magnitude 16".
Physical Information: Apparent size 0.8 by 0.4? arcmin.

IC 5206 (= PGC 68762)
Discovered (Aug 21, 1900) by DeLisle Stewart
A magnitude 14.5 spiral galaxy (type SBbc??) in Tucana (RA 22 24 04.5, Dec -66 51 28)

Historical Identification: Per Dreyer, IC 5206 (DeLisle Stewart #749, 1860 RA 22 13 48, NPD 157 33) is "extremely faint, very small, round, stellar nucleus".
Physical Information: Apparent size 0.9 by 0.6? arcmin.

IC 5207 (= PGC 68738)
Discovered (Jul 16, 1904) by Royal Frost
A magnitude 14.5 spiral galaxy (type SBc??) in Tucana (RA 22 23 29.2, Dec -60 33 56)

Historical Identification: Per Dreyer, IC 5207 (Frost #1228, 1860 RA 22 13 56, NPD 151 17) has a "brighter middle, magnitude 16".
Physical Information: Apparent size 1.5 by 0.9? arcmin.

IC 5208 (= PGC 68788)
Discovered (Aug 21, 1900) by DeLisle Stewart
A magnitude 13.8 lenticular galaxy (type S0/a??) in Tucana (RA 22 24 34.1, Dec -65 13 39)

Historical Identification: Per Dreyer, IC 5208 (DeLisle Stewart #751, 1860 RA 22 14 29, NPD 155 55) is "most extremely faint, extremely small, extremely extended 65�, stellar nucleus".
Physical Information: Apparent size 1.6 by 0.2? arcmin.

IC 5209 (= PGC 68722)
Discovered (1899) by DeLisle Stewart
A magnitude 14.8 spiral galaxy (tpe Sc??) in Grus (RA 22 23 09.1, Dec -37 59 37)

Historical Identification: Per Dreyer, IC 5209 (DeLisle Stewart #750, 1860 RA 22 14 50, NPD 128 41) is "faint, extremely small, round, 2 stars to northwest".
Physical Information: Apparent size 0.6 by 0.5? arcmin.

IC 5210 (= PGC 68674)
Discovered (Aug 8, 1896) by Lewis Swift
Also observed (1899?) by Herbert Howe
A magnitude 13.0 lenticular galaxy (type E/S0??) in Aquarius (RA 22 22 31.1, Dec -18 52 09)

Historical Identification: Per Dreyer, IC 5210 (Swift list XI (#213), Howe, 1860 RA 22 14 53, NPD 109 34.4) is "most extremely faint, very small, round, preceding (western) of 2", the other being IC 5211.
Discovery Notes: It appears that Swift accidentally reversed the descriptions of his #213 and 214, placing the description of the western galaxy with the entry for the eastern one, and vice-versa. Dreyer must have used Howe's observations to correct the positions and positional description, but did not correct Swift's physical/field descriptions, which should have read "most extremely faint, very small, round" for IC 5211, and "extremely faint, small, north of and near to easternmost star of 7 in an east-west line" for IC 5210.
Physical Information: Apparent size 1.2 by 1.1? arcmin.

IC 5211 (= PGC 68695)
Discovered (Jun 8, 1896) by Lewis Swift
Also observed (1899?) by Herbert Howe
A magnitude 13.5 spiral galaxy (type Sab??) in Aquarius (RA 22 22 42.9, Dec -18 52 47)

Historical Identification: Per Dreyer, IC 5211 (Swift list XI (#214), Howe, 1860 RA 22 15 05, NPD 109 35.1) is "extremely faint, small, following (eastern) of 2", the other being IC 5210
Discovery Notes: It appears that Swift accidentally reversed the descriptions of his #213 and 214, placing the description of the western galaxy with the entry for the eastern one, and vice-versa. Dreyer must have used Howe's observations to correct the positions and positional description, but did not correct Swift's physical/field descriptions, which should have read "most extremely faint, very small, round" for IC 5211, and "extremely faint, small, north of and near to easternmost star of 7 in an east-west line" for IC 5210.
Physical Information: Apparent size 1.0 by 0.6? arcmin.

IC 5212 (= PGC 68739)
Discovered (1899) by DeLisle Stewart
A magnitude 13.5 spiral galaxy (tpe Sc??) in Grus (RA 22 23 30.2, Dec -38 02 16)

Historical Identification: Per Dreyer, IC 5212 (DeLisle Stewart #752, 1860 RA 22 15 14, NPD 128 45) is "extremely faint, extremely small, considerably extended 40�".
Physical Information: Apparent size 1.1 by 0.7? arcmin.

IC 5213 (= PGC 68809)
Discovered (Jul 16, 1904) by Royal Frost
A magnitude 15.0 spiral galaxy (type Sc??) in Tucana (RA 22 25 04.9, Dec -60 28 34)

Historical Identification: Per Dreyer, IC 5213 (Frost #1229, 1860 RA 22 15 27, NPD 151 11) has a "brighter middle, magnitude 16".
Physical Information: Apparent size 0.6 by 0.5? arcmin.

IC 5214 (= PGC 68694)
Discovered (Jul 26, 1897) by Lewis Swift
A magnitude 14.4 spiral galaxy (type Sc??) in Piscis Austrinus (RA 22 22 43.4, Dec -27 21 20)

Historical Identification: Per Dreyer, IC 5214 (Swift list XII (#37), 1860 RA 22 15 50, NPD 118 10.6) is "extremely faint, pretty small, round, 8th magnitude star to west".
Physical Information: Apparent size 1.0 by 0.2? arcmin.

IC 5215 (= PGC 68888)
Discovered (Aug 21, 1900) by DeLisle Stewart
A magnitude 14.9 spiral galaxy (type Sc??) in Tucana (RA 22 26 58.0, Dec -65 58 58)

Historical Identification: Per Dreyer, IC 5215 (DeLisle Stewart #753, 1860 RA 22 16 52, NPD 156 39) is "extremely faint, very small, round, star 2 arcmin to northeast; suspected".
Physical Information: Apparent size 0.6 by 0.5? arcmin.

IC 5216
Recorded (Jun 9, 1896) by Stephane Javelle
A lost or nonexistent object in Aquarius (RA 22 24 44.0, Dec -18 05 18)

Historical Identification: Per Dreyer, IC 5216 (Javelle #1416, 1860 RA 22 17 08, NPD 108 47.7) is "very faint, small, round, nuclear".

IC 5217
Discovered (1904) by Williamina Fleming
A magnitude 11.3 planetary nebula in Lacerta (RA 22 23 55.7, Dec +50 58 03)

Historical Identification: Per Dreyer, IC 5217 (Fleming #102, 1860 RA 22 18 18, NPD 39 44) is "planetary, stellar".
Physical Information: Apparent size 0.25? arcmin.

IC 5218 (= PGC 68927)
Discovered (Jul 16, 1904) by Royal Frost
A magnitude 14.3 spiral galaxy (type SBbc??) in Tucana (RA 22 28 05.8, Dec -60 23 41)

Historical Identification: Per Dreyer, IC 5218 (Frost #1230, 1860 RA 22 18 40, NPD 151 06) is "faint, pretty small, extended 195�".
Physical Information: Apparent size 1.3 by 0.5? arcmin.

IC 5219 (= PGC 68955)
Discovered (Aug 21, 1900) by DeLisle Stewart
A magnitude 15.1 spiral galaxy (type Sc??) in Tucana (RA 22 28 44.1, Dec -65 53 37)

Historical Identification: Per Dreyer, IC 5219 (DeLisle Stewart #754, 1860 RA 22 18 41, NPD 156 35) is "extremely faint, extremely small, considerably extended 15�, suspected".
Physical Information: Apparent size 0.8 by 0.5? arcmin.

IC 5220 (= PGC 68925)
Discovered (Jul 16, 1904) by Royal Frost
A magnitude 14.3 spiral galaxy (type Sc??) in Tucana (RA 22 28 02.4, Dec -59 43 22)

Historical Identification: Per Dreyer, IC 5220 (Frost #1231, 1860 RA 22 18 48, NPD 150 26) is "faint, pretty small, extended 105�".
Physical Information: Apparent size 1.1 by 0.3? arcmin.

IC 5221 (= PGC 68967)
Discovered (Aug 21, 1900) by DeLisle Stewart
A magnitude 14.9 elliptical galaxy (type E2??) in Tucana (RA 22 28 57.9, Dec -65 54 15)

Historical Identification: Per Dreyer, IC 5221 (DeLisle Stewart #755, 1860 RA 22 18 53, NPD 156 36) is "extremely faint, brighter middle, suspected".
Physical Information: Apparent size 0.5 by 0.4? arcmin.

IC 5222 (= PGC 68993)
Discovered (Aug 21, 1900) by DeLisle Stewart
A magnitude 12.8 spiral galaxy (type SBbc??) in Tucana (RA 22 29 54.7, Dec -65 39 41)

Historical Identification: Per Dreyer, IC 5222 (DeLisle Stewart #756, 1860 RA 22 19 54, NPD 156 21) is "a remarkable object, extremely faint, pretty small, stellar nucleus, suspected".
Physical Information: Apparent size 1.9 by 1.3? arcmin.

IC 5223 (= PGC 68988)
Discovered (Oct 23, 1903) by Stephane Javelle
A magnitude 14.6 lenticular galaxy (type S0/a??) in Pegasus (RA 22 29 44.8, Dec +07 59 19)

Historical Identification: Per Dreyer, IC 5223 (Javelle #1417, 1860 RA 22 22 44, NPD 82 43.2) is "faint, very small, diffuse, mottled but not resolved".
Physical Information: Apparent size 1.0 by 0.3? arcmin. Steinicke lists as three galaxies, but the second and third are too faint to be part of the IC object, and the third is almost certainly a completely unrelated object.

IC 5224 (= PGC 69011)
Discovered (1900) by Joseph Lunt
A magnitude 13.6 spiral galaxy (type Sab??) in Grus (RA 22 30 30.0, Dec -45 59 45)

Historical Identification: Per Dreyer, IC 5224 (Lunt (#5), 1860 RA 22 23 04, NPD 136 42.2) has "no description".
Physical Information: Apparent size 1.5 by 0.4? arcmin.

IC 5225 (= NGC 7294 = PGC 69088)
Discovered (1886) by Francis Leavenworth (and later listed as NGC 7294)
Discovered (Oct 6, 1897) by Lewis Swift (and later listed as IC 5225)
A magnitude 12.5 lenticular galaxy (type SB0??) in Piscis Austrinus (RA 22 32 07.8, Dec -25 23 53)

Historical Identification: Per Dreyer, IC 5225 (Swift list XII (#38), 1860 RA 22 23 47, NPD 116 04.9) is "most extremely faint, pretty small, round, between 2 stars".
Physical Information: Given the duplicate entry, see NGC 7294 for anything else.

IC 5226 (= PGC 69097)
Discovered (Oct 6, 1897) by Lewis Swift
A magnitude 12.6 spiral galaxy (type SBc??) in Piscis Austrinus (RA 22 32 30.0, Dec -25 39 44)

Historical Identification: Per Dreyer, IC 5226 (Swift list XII (#39), 1860 RA 22 23 57, NPD 115 22.6) is "most extremely faint, pretty large, round".
Physical Information: Apparent size 2.6 by 2.4? arcmin.

IC 5227 (= PGC 69170)
Discovered (Aug 21, 1900) by DeLisle Stewart
A magnitude 13.1 spiral galaxy (type SBab??) in Tucana (RA 22 34 03.6, Dec -64 41 52)

Historical Identification: Per Dreyer, IC 5227 (DeLisle Stewart #757, 1860 RA 22 24 22, NPD 155 24) is "faint, small, stellar nucleus".
Physical Information: Apparent size 1.4 by 1.0? arcmin.

IC 5228 (= NGC 7302 = PGC 69094)
Discovered (Oct 3, 1785) by William Herschel (and later listed as NGC 7302)
Discovered (Aug 8, 1896) by Lewis Swift (and later listed as IC 5228)
A magnitude 12.3 lenticular galaxy (type E/S0??) in Aquarius (RA 22 32 23.9, Dec -14 07 15)

Historical Identification: Per Dreyer, IC 5228 (Swift list XI (#215), 1860 RA 22 24 46, NPD 104 50.4) is "pretty bright, pretty small, round, bright star to south".
Physical Information: Given the duplicate entry, see NGC 7302 for anything else.

IC 5229 (= PGC 69217)
Discovered (Jul 16, 1904) by Royal Frost
A magnitude 14.4 spiral galaxy (type Sc??) in Tucana (RA 22 34 50.3, Dec -61 22 52)

Historical Identification: Per Dreyer, IC 5229 (Frost #1232, 1860 RA 22 25 24, NPD 152 06) has a "brighter middle, magnitude 15".
Physical Information: Apparent size 0.7 by 0.7? arcmin.

IC 5230 (= PGC 69249)
Discovered (1899) by DeLisle Stewart
A magnitude 14.3 spiral galaxy (type Sc??) in Tucana (RA 22 25 40.2, Dec -61 32 50)

Historical Identification: Per Dreyer, IC 5230 (DeLisle Stewart #758, 1860 RA 22 26 12, NPD 152 15) is "extremely faint, extremely small, considerably extended 35�, considerably brighter middle".
Physical Information: Apparent size 1.1 by 0.4? arcmin.

IC 5231 (= PGC 69166)
Discovered (Oct 9, 1895) by Stephane Javelle
A magnitude 14.5 lenticular galaxy (type S0/a??) in Pegasus (RA 22 34 00.6, Dec +23 20 21)

Historical Identification: Per Dreyer, IC 5231 (Javelle #1418, 1860 RA 22 27 20, NPD 67 23.0) is "faint, small, round, gradually brighter middle and nucleus".
Physical Information: Apparent size 1.0 by 0.9? arcmin.

IC 5232 (= PGC 69358)
Discovered (Aug 21, 1900) by DeLisle Stewart
A magnitude 14.6 spiral galaxy (type Sc??) in Indus (RA 22 37 38.3, Dec -68 52 17)

Historical Identification: Per Dreyer, IC 5232 (DeLisle Stewart #759, 1860 RA 22 27 32, NPD 159 35) is "extremely faint, most extremely small, brighter middle".
Physical Information: Apparent size 0.7 by 0.3? arcmin.

IC 5233 (= PGC 69290)
Discovered (Oct 13, 1903) by Stephane Javelle
A magnitude 13.8 spiral galaxy (type Sbc??) in Pegasus (RA 22 36 33.0, Dec +25 45 49)

Historical Identification: Per Dreyer, IC 5233 (Javelle #1419, 1860 RA 22 29 56, NPD 64 58.4) is "faint, very small, diffuse, 12.5 magnitude star very close".
Physical Information: Apparent size 1.0 by 0.8? arcmin.

IC 5234 (= PGC 69446)
Discovered (Aug 21, 1900) by DeLisle Stewart
A magnitude 14.4 lenticular galaxy (type S0/a??) in Tucana (RA 22 40 11.4, Dec -65 49 29)

Historical Identification: Per Dreyer, IC 5234 (DeLisle Stewart #760, 1860 RA 22 30 29, NPD 156 32) is "extremely faint, most extremely small, considerably extended 165�, considerably brighter middle".
Physical Information: Apparent size 1.0 by 0.4? arcmin.

IC 5235 (= PGC 69497)
Discovered (Aug 21, 1900) by DeLisle Stewart
A magnitude 12.6 lenticular galaxy (type S0/a??) in Tucana (RA 22 41 25.6, Dec -66 34 49)

Historical Identification: Per Dreyer, IC 5235 (DeLisle Stewart #761, 1860 RA 22 31 40, NPD 157 18) is "most extremely faint, brighter middle".
Physical Information: Apparent size 0.5 by 0.4? arcmin.

IC 5236 (= PGC 69503)
Discovered (Aug 21, 1900) by DeLisle Stewart
A magnitude 14.4 lenticular galaxy (type S0??) in Tucana (RA 22 41 30.4, Dec -66 37 04)

Historical Identification: Per Dreyer, IC 5236 (DeLisle Stewart #762, 1860 RA 22 31 46, NPD 157 20) is "extremely faint, most extremely small, considerably extended 60�, brighter middle".
Physical Information: Apparent size 0.8 by 0.4? arcmin.

IC 5237 (= NGC 7361 = PGC 69539)
Discovered (Sep 28, 1834) by John Herschel (and later listed as NGC 7361)
Discovered (Jul 19, 1897) by Lewis Swift (and later listed as IC 5237)
A magnitude 12.3 spiral galaxy (type Sc??) in Piscis Austrinus (RA 22 42 17.9, Dec -30 03 27)

Historical Identification: Per Dreyer, IC 5237 (Swift list XII (#40), 1860 RA 22 32 06, NPD 120 44.0) is "most extremely faint, extremely small, extremely extended, 8th magnitude star to northwest".
Physical Information: Given the duplicate entry, see NGC 7361 for anything else.

IC 5238 (= PGC 69501)
Discovered (Jul 16, 1904) by Royal Frost
A magnitude 15.0 spiral galaxy (type Sc??) in Tucana (RA 22 41 29.9, Dec -60 45 28)

Historical Identification: Per Dreyer, IC 5238 (Frost #1233, 1860 RA 22 32 21, NPD 151 29) is "faint, very small, very little extended".
Physical Information: Apparent size 0.8 by 0.3? arcmin.

IC 5239
Recorded (Jul 7, 1897) by Lewis Swift
A lost or nonexistent object in Grus (RA 22 40 45.0, Dec -38 02 36)

Historical Identification: Per Dreyer, IC 5239 (Swift list XI (#216), 1860 RA 22 32 41, NPD 128 46.2) is "very faint, pretty small, round".

IC 5240 (= PGC 69521)
Discovered (Dec 26, 1886) by William Finlay
Also observed (Aug 8, 1897) by Lewis Swift
A magnitude 11.9 spiral galaxy (type SBa??) in Grus (RA 22 41 52.1, Dec -44 46 01)

Historical Identification: Per Dreyer, IC 5240 (Finlay (#12), Swift list XI (#217), 1860 RA 22 33 38, NPD 135 31.7) is "pretty faint, pretty large, round, faint star to southeast".
Physical Information: Apparent size 2.8 by 1.8? arcmin.

IC 5241 (= PGC 69504)
Discovered (Oct 16, 1903) by Stephane Javelle
A magnitude 13.9 spiral galaxy (type SBc??) in Aquarius (RA 22 41 38.5, Dec +02 38 23)

Historical Identification: Per Dreyer, IC 5241 (Javelle #1420, 1860 RA 22 34 30, NPD 88 05.3) is "pretty bright, considerably small, round, gradually brighter middle, mottled but not resolved".
Physical Information: Apparent size 1.0 by 0.8? arcmin.

IC 5242 (= PGC 69487)
Discovered (Nov 9, 1896) by Stephane Javelle
A magnitude 13.7 spiral galaxy (type Sab??) in Pegasus (RA 22 41 15.1, Dec +23 24 25)

Historical Identification: Per Dreyer, IC 5242 (Javelle #1421, 1860 RA 22 34 30, NPD 67 19.8) is "faint, small, round, gradually brighter middle, 13th magnitude star to northeast".
Physical Information: Apparent size 0.8 by 0.8? arcmin.

IC 5243 (= PGC 69495)
Discovered (Nov 9, 1896) by Stephane Javelle
A magnitude 14.5 spiral galaxy (type Sbc??) in Pegasus (RA 22 41 24.5, Dec +23 22 32)

Historical Identification: Per Dreyer, IC 5243 (Javelle #1422, 1860 RA 22 34 40, NPD 67 21.7) is "faint, considerably small, irregular figure, diffuse".
Physical Information: Apparent size 0.7 by 0.6? arcmin. Steinicke states a double system.

IC 5244 (= PGC 69620)
Discovered (1899) by DeLisle Stewart
A magnitude 12.6 spiral galaxy (type Sb??) in Tucana (RA 22 44 13.5, Dec -64 02 35)

Historical Identification: Per Dreyer, IC 5244 (DeLisle Stewart #763, 1860 RA 22 34 53, NPD 154 45) is "extremely faint, pretty small, extremely extended 0�, stellar nucleus".
Physical Information: Apparent size 3.0 by 0.4? arcmin.

IC 5245 (= PGC 69645)
Discovered (Aug 21, 1900) by DeLisle Stewart
A magnitude 14.2 lenticular galaxy (type S0/a??) in Tucana (RA 22 44 56.6, Dec -65 21 27)

Historical Identification: Per Dreyer, IC 5245 (DeLisle Stewart #764, 1860 RA 22 35 33, NPD 156 04) is "extremely faint, extremely small, round, faint star 0.5 arcmin to northwest".
Physical Information: Apparent size 0.8 by 0.7? arcmin.

IC 5246 (= PGC 69696)
Discovered (Aug 21, 1900) by DeLisle Stewart
A magnitude 13.8 spiral galaxy (type Sc??) in Tucana (RA 22 46 39.5, Dec -64 53 52)

Historical Identification: Per Dreyer, IC 5246 (DeLisle Stewart #765, 1860 RA 22 37 10, NPD 155 38) is "extremely faint, extremely small".
Physical Information: Apparent size 1.0 by 0.6? arcmin.

IC 5247 (= PGC 69700)
Discovered (Aug 21, 1900) by DeLisle Stewart
A magnitude 13.9 spiral galaxy (type Sc??) in Tucana (RA 22 46 49.9, Dec -65 16 25)

Historical Identification: Per Dreyer, IC 5247 (DeLisle Stewart #766, 1860 RA 22 37 28, NPD 156 01) is "very faint, very small, much extended 125�, much brighter middle".
Physical Information: Apparent size 1.3 by 0.4? arcmin.

IC 5248
Recorded (Dec 6, 1888) by Guillaume Bigourdan
A lost or nonexistent object in Aquarius (RA 22 44 42.7, Dec -00 20 32)

Historical Identification: Per Dreyer, IC 5248 (Bigourdan #347, 1860 22 37 31, NPD 91 05) is "suspected (13.5 magnitude)".

IC 5249 (= PGC 69707)
Discovered (Aug 21, 1900) by DeLisle Stewart
A magnitude 13.6 spiral galaxy (type SBcd??) in Tucana (RA 22 47 06.4, Dec -64 49 50)

Historical Identification: Per Dreyer, IC 5249 (DeLisle Stewart #767, 1860 RA 22 37 47, NPD 155 34) is "extremely faint, very small, extremely extended 15�, very little brighter middle".
Physical Information: Apparent size 3.6 by 0.4? arcmin.