40:
1823:
233:
1824:
G. D. Banks, M. J. Disney, P. M. Knezek, H. Jerjen, D. G. Barnes, R. Bhatal, W. J. G. de Blok, P. J. Boyce, R. D. Ekers, K. C. Freeman, B. K. Gibson, P. A. Henning, V. Kilborn, B. Koribalski, R. C. Kraan-Korteweg, D. F. Malin, R. F. Minchin, J. R. Mould, T. Oosterloo, R. M. Price, M. E. Putman, S. D.
278:
survey, which was a more intensive radio survey for hydrogen emission within a smaller region of the sky. Several optical surveys later identified 20 more candidate objects to the group. In 2007, the Cen A group membership of NGC 5011C was established. While this galaxy is a well-known stellar
1892:
R. F. Minchin, M. J. Disney, P. J. Boyce, W. J. G. de Blok, Q. A. Parker, G. D. Banks, K. C. Freeman, D. A. Garcia, B. K. Gibson, M. Grossi, R. F. Haynes, P. M. Knezek, R. H. Lang, D. F. Malin, R. M. Price, I. M. Stewart, A. E. Wright (2003). "HIDEEP - an extragalactic blind survey for very low
240:
The brightest group members were frequently identified in early galaxy group identification surveys. However, many of the dwarf galaxies in the group were only identified in more intensive studies. One of the first of these identified 145 faint objects on optical images from the
1891:
273:
survey, which was a blind radio survey for hydrogen spectral line emission, found five uncatalogued galaxies in the group and also identified five previously-catalogued galaxies as members. An additional dwarf galaxy was identified as a group member in the
2250:
Müller, Oliver; Fahrion, Katja; Rejkuba, Marina; Hilker, Michael; Lelli, Federico; Lutz, Katharina; Pawlowski, Marcel S.; Coccato, Lodovico; Anand, Gagandeep S.; Jerjen, Helmut (2021). "The properties of dwarf spheroidal galaxies in the Cen a group".
279:
system listed with a NGC number, its true identity remained hidden because of coordinate confusion and wrong redshifts in the literature. From 2015 to 2017 a full optical survey was conducted using the
2296:
M. Grossi; M. J. Disney; B. J. Pritzl; P. M. Knezek; J. S. Gallagher; R. F. Minchin; K. C> Freeman (2007). "Star formation history and evolution of gas-rich dwarf galaxies in the
Centaurus A group".
1825:
Ryder, E. M. Sadler, L. Staveley-Smith, I. Stewart, F. Stootman, R. A. Vaile, R. L. Webster, A. E. Wright (1999). "New
Galaxies Discovered in the First Blind H I Survey of the Centaurus A Group".
1490:
is only listed as a possible member of the M83 Subgroup in the later list published by
Karachentsev, later analyses indicate that this galaxy is within the subgroup. Saviane and Jerjen found that
208:. However, the galaxies around Centaurus A and the galaxies around M83 are physically close to each other, and both subgroups appear not to be moving relative to each other.
2173:
Müller, Oliver, Helmut Jerjen, and Bruno
Binggeli. “New Low Surface Brightness Dwarf Galaxies in the Centaurus Group.” Astronomy & Astrophysics 597 (January 2017): A7.
2160:
Müller, Oliver, Helmut Jerjen, and Bruno
Binggeli. “New Dwarf Galaxy Candidates in the Centaurus Group.” Astronomy & Astrophysics 583 (November 2015): A79.
2063:
I. D. Karachentsev; M. E. Sharina; A. E. Dolphin; E. K. Grebel; D. Geisler; P. Guhathakurta; P. W. Hodge; V. E. Karachetseva; A. Sarajedini; P. Seitzer (2002).
1494:
has an optical redshift of 647 km/s and thus is a member of the Cen A group rather than of the distant
Centaurus galaxy cluster as believed since 1983.
1966:
H. Jerjen; K. C. Freeman; B. Binggeli (2000). "Testing the
Surface Brightness Fluctuations Method for Dwarf Elliptical Galaxies in the Centaurus A Group".
307:
1176:
283:, covering 550 square degrees in the sky and doubling the number of known dwarf galaxies in this group. Another deep but spatially limited survey around
1895:
1487:
1153:
1130:
537:
514:
490:
467:
444:
200:
This group is sometimes identified as one group and sometimes identified as two groups. Hence, some references will refer to two objects named the
1948:
1878:
1692:
P. Fouque; E. Gourgoulhon; P. Chamaraux; G. Paturel (1992). "Groups of galaxies within 80 Mpc. II - The catalogue of groups and group members".
1475:
1463:
1295:
1271:
1106:
721:
698:
675:
652:
628:
1491:
1483:
1471:
1467:
1413:
1390:
1028:
1004:
981:
957:
934:
910:
886:
862:
840:
1437:
816:
792:
298:, and follow a similar metallicity–luminosity relation. One dwarf galaxy, KK98 203 (LEDA 166167), has an extended ring of Hα emission.
1771:
S. Cote; K. C. Freeman; C. Carigan; P. J. Quinn (1997). "Discovery of
Numerous Dwarf Galaxies in the Two Nearest Groups of Galaxies".
1223:
1199:
1247:
605:
582:
559:
294:
of the
Centaurus A group have been studied and have been found to have old, metal-poor stellar populations similar to those in the
275:
397:
374:
2350:
1952:
1064:
332:
1673:
1520:
2021:"Surface BR Photometry of Newly Discovered Dwarf Elliptical Galaxies in the Nearby Sculptor and Centaurus A Groups"
2370:
262:
1083:
1073:
351:
341:
306:
The table below lists galaxies that have been identified as associated with the
Centaurus A/M83 Group by
1665:
2191:; Caldwell, N.; Guhathakurta, P.; McLeod, B.; Seth, A.; Simon, J. D.; Strader, J.; Toloba, E. (2016).
291:
2375:
133:
165:. The group may be roughly divided into two subgroups. The Cen A Subgroup, at a distance of 11.9
250:
21:
2344:
1942:
1872:
310:
and collaborators. Note that Karachentsev divides this group into two subgroups centered on
162:
154:
129:
77:
69:
2080:
1732:
1719:
A. Garcia (1993). "General study of group membership. II - Determination of nearby groups".
1705:
2316:
2214:
2127:
2076:
2032:
1985:
1914:
1844:
1790:
1728:
1701:
1623:
242:
8:
2320:
2218:
2131:
2062:
2036:
1989:
1918:
1848:
1794:
1627:
2332:
2306:
2278:
2260:
2232:
2204:
2143:
2117:
2001:
1975:
1930:
1904:
1860:
1834:
1806:
1780:
1639:
1613:
1099:
367:
280:
212:
2105:
2328:
2282:
2236:
2227:
2193:"The Extended Halo of Centaurus A: Uncovering Satellites, Streams, and Substructures"
2192:
2188:
1934:
1926:
1864:
1810:
1669:
1643:
1516:
55:
17:
2336:
2147:
2005:
2324:
2270:
2222:
2135:
2084:
2040:
1993:
1922:
1852:
1798:
1631:
2274:
1746:
1604:
I. D. Karachentsev (2005). "The Local Group and Other Neighboring Galaxy Groups".
2089:
2064:
1069:
337:
84:
2174:
2161:
2364:
2295:
1691:
258:
246:
194:
151:
63:
236:
The galaxies NGC 5011B and NGC 5011C are imaged against a starry foreground.
266:
178:
147:
2311:
2122:
1980:
1909:
1839:
1785:
1770:
1618:
1079:
419:
347:
311:
295:
284:
216:
174:
109:
96:
45:
39:
1318:
315:
190:
182:
166:
1474:
are listed as possibly being members of the Centaurus A Subgroup, and
158:
73:
1486:
are listed as possibly being members of the M83 Subgroup. Although
2265:
2209:
2139:
2045:
2020:
1997:
1856:
1802:
1635:
1479:
1366:
1342:
1089:
768:
744:
357:
254:
1565:
27:
Group of galaxies in the constellations Centaurus, Hydra and Virgo
2018:
1965:
2106:"NGC 5011C: An Overlooked Dwarf Galaxy in the Centaurus A Group"
1093:
361:
270:
186:
170:
2186:
232:
2249:
48:
galaxy is the largest and most massive galaxy in the group
2058:
2056:
2065:"New distances to galaxies in the Centaurus A group"
2053:
1510:
2103:
1603:
1599:
1597:
1595:
1593:
1591:
1589:
1587:
1585:
2299:Monthly Notices of the Royal Astronomical Society
1896:Monthly Notices of the Royal Astronomical Society
2362:
1687:
1685:
1959:
1885:
1582:
2019:H. Jerjen; K. C. Freeman; B. Binggeli (2000).
1511:Kepple, George Robert; Glen W. Sanner (1998).
1682:
1947:: CS1 maint: multiple names: authors list (
1877:: CS1 maint: multiple names: authors list (
1817:
2175:https://doi.org/10.1051/0004-6361/201628921
2162:https://doi.org/10.1051/0004-6361/201526748
2012:
1764:
1659:
181:. The M83 Subgroup, at a distance of 14.9
2289:
875:−46° 59′ 27.3″
549:−46° 58′ 12.9″
2310:
2264:
2226:
2208:
2121:
2088:
2044:
1979:
1908:
1838:
1784:
1718:
1712:
1617:
211:The Centaurus A/M83 Group is part of the
1513:The Night Sky Observer's Guide, Volume 2
1450:−29° 14′ 06″
1426:−28° 02′ 42″
1402:−30° 07′ 03″
1379:−29° 54′ 47″
1355:−31° 38′ 24″
1331:−29° 51′ 57″
1308:−33° 34′ 22″
1284:−31° 31′ 45″
1260:−29° 34′ 17″
1236:−28° 53′ 32″
1212:−30° 21′ 45″
1188:−33° 21′ 23″
1166:−29° 58′ 41″
1143:−31° 53′ 11″
1119:−30° 58′ 19″
1041:−35° 19′ 59″
1017:−41° 51′ 40″
994:−45° 12′ 18″
970:−41° 28′ 50″
947:−42° 32′ 07″
923:−45° 03′ 42″
899:−44° 53′ 24″
853:−46° 35′ 06″
829:−42° 50′ 49″
805:−48° 09′ 04″
781:−36° 37′ 49″
757:−49° 28′ 06″
734:−46° 59′ 46″
711:−45° 41′ 05″
688:−43° 46′ 11″
665:−45° 21′ 10″
641:−40° 04′ 58″
618:−42° 34′ 55″
595:−42° 43′ 41″
572:−42° 56′ 23″
526:−37° 58′ 29″
503:−39° 53′ 48″
480:−36° 19′ 44″
457:−41° 49′ 57″
433:−43° 01′ 09″
409:−47° 33′ 54″
387:−38° 53′ 56″
231:
227:
2363:
2097:
1560:
1558:
1556:
1554:
1552:
215:, the local supercluster of which the
1721:Astronomy and Astrophysics Supplement
1694:Astronomy and Astrophysics Supplement
1655:
1653:
1550:
1548:
1546:
1544:
1542:
1540:
1538:
1536:
1534:
1532:
1504:
323:Members of the Centaurus A Subgroup
13:
2349:: CS1 maint: unflagged free DOI (
1893:column-density neutral hydrogen".
1650:
1566:"NASA/IPAC Extragalactic Database"
1529:
1515:. Willmann-Bell, Inc. p. 73.
14:
2387:
1951:) CS1 maint: unflagged free DOI (
2329:10.1111/j.1365-2966.2006.11125.x
1927:10.1111/j.1365-2966.2003.07134.x
38:
2243:
2180:
2167:
2154:
132:5128 Group, Centaurus A Group,
2104:I. Saviane; H. Jerjen (2007).
1751:ESA/Hubble Picture of the Week
1739:
301:
287:revealed numerous new dwarfs.
269:as members of the group. The
1:
1497:
263:Siding Spring 2.3 m Telescope
2253:Astronomy & Astrophysics
2187:Crnojević, D.; Sand, D. J.;
7:
2275:10.1051/0004-6361/202039359
1055:Members of the M83 Subgroup
10:
2392:
2228:10.3847/0004-637X/823/1/19
2090:10.1051/0004-6361:20020042
2069:Astronomy and Astrophysics
1666:Cambridge University Press
1570:Results for NGC 5128 Group
222:
15:
2197:The Astrophysical Journal
292:dwarf spheroidal galaxies
245:and followed these up in
128:
123:
115:
105:
95:
83:
62:
53:
37:
32:
2025:The Astronomical Journal
101:−44° 58′
16:Not to be confused with
2081:2002A&A...385...21K
1747:"Don't trust your eyes"
1733:1993A&AS..100...47G
1706:1992A&AS...93..211F
1662:Nearby Galaxies Catalog
219:is an outlying member.
189:), is centered on the
265:. This identified 20
251:Parkes Radio Telescope
237:
22:Centaurus Supercluster
2371:Centaurus A/M83 Group
1827:Astrophysical Journal
235:
228:Member identification
144:Centaurus A/M83 Group
33:Centaurus A/M83 group
2110:Astronomical Journal
1968:Astronomical Journal
1773:Astronomical Journal
1660:R. B. Tully (1988).
1606:Astronomical Journal
243:UK Schmidt Telescope
2321:2007MNRAS.374..107G
2219:2016ApJ...823...19C
2132:2007AJ....133.1756S
2037:2000AJ....119..593J
1990:2000AJ....119..166J
1919:2003MNRAS.346..787M
1849:1999ApJ...524..612B
1795:1997AJ....114.1313C
1628:2005AJ....129..178K
1057:
325:
1100:Apparent Magnitude
1053:
368:Apparent Magnitude
321:
308:I. D. Karachentsev
281:Dark Energy Camera
249:emission with the
238:
213:Virgo Supercluster
173:), is centered on
124:Other designations
116:Number of galaxies
54:Observation data (
1460:
1459:
1177:HIDEEP J1336-3321
1051:
1050:
202:Centaurus A Group
193:(M83), a face-on
148:group of galaxies
140:
139:
18:Centaurus Cluster
2383:
2355:
2354:
2348:
2340:
2314:
2312:astro-ph/0611106
2293:
2287:
2286:
2268:
2247:
2241:
2240:
2230:
2212:
2184:
2178:
2171:
2165:
2158:
2152:
2151:
2125:
2123:astro-ph/0701280
2116:(4): 1756–1762.
2101:
2095:
2094:
2092:
2060:
2051:
2050:
2048:
2016:
2010:
2009:
1983:
1981:astro-ph/9912011
1963:
1957:
1956:
1946:
1938:
1912:
1910:astro-ph/0308405
1889:
1883:
1882:
1876:
1868:
1842:
1840:astro-ph/9906146
1821:
1815:
1814:
1788:
1786:astro-ph/9704030
1768:
1762:
1761:
1759:
1757:
1743:
1737:
1736:
1716:
1710:
1709:
1689:
1680:
1679:
1657:
1648:
1647:
1621:
1619:astro-ph/0410065
1601:
1580:
1579:
1577:
1576:
1562:
1527:
1526:
1508:
1447:
1423:
1399:
1376:
1352:
1328:
1305:
1281:
1257:
1233:
1209:
1185:
1163:
1140:
1116:
1058:
1052:
1038:
1014:
991:
967:
944:
920:
896:
872:
850:
826:
802:
778:
754:
731:
708:
685:
662:
638:
615:
592:
569:
546:
523:
500:
477:
454:
430:
406:
384:
326:
320:
106:Brightest member
91:
42:
30:
29:
2391:
2390:
2386:
2385:
2384:
2382:
2381:
2380:
2376:Galaxy clusters
2361:
2360:
2359:
2358:
2342:
2341:
2294:
2290:
2248:
2244:
2185:
2181:
2172:
2168:
2159:
2155:
2102:
2098:
2061:
2054:
2017:
2013:
1964:
1960:
1940:
1939:
1890:
1886:
1870:
1869:
1822:
1818:
1769:
1765:
1755:
1753:
1745:
1744:
1740:
1717:
1713:
1690:
1683:
1676:
1658:
1651:
1602:
1583:
1574:
1572:
1564:
1563:
1530:
1523:
1509:
1505:
1500:
1488:HIPASS J1337-39
1445:
1421:
1397:
1374:
1350:
1326:
1303:
1279:
1255:
1231:
1207:
1183:
1161:
1154:Centaurus A-dE4
1138:
1131:Centaurus A-dE2
1114:
1036:
1012:
989:
965:
942:
918:
894:
870:
848:
824:
800:
776:
752:
729:
706:
683:
660:
636:
613:
590:
567:
544:
538:HIPASS J1351-47
521:
515:HIPASS J1348-37
498:
491:HIPASS J1337-39
475:
468:Centaurus A-dE3
452:
445:Centaurus A-dE1
428:
404:
382:
304:
230:
225:
89:
85:Right ascension
49:
28:
25:
12:
11:
5:
2389:
2379:
2378:
2373:
2357:
2356:
2305:(1): 107–130.
2288:
2242:
2179:
2166:
2153:
2140:10.1086/512157
2096:
2052:
2046:10.1086/301216
2031:(2): 593–608.
2011:
1998:10.1086/301188
1974:(1): 166–176.
1958:
1903:(3): 787–802.
1884:
1857:10.1086/307854
1833:(2): 612–622.
1816:
1803:10.1086/118565
1763:
1738:
1711:
1681:
1674:
1649:
1636:10.1086/426368
1612:(1): 178–188.
1581:
1528:
1521:
1502:
1501:
1499:
1496:
1462:Additionally,
1458:
1457:
1454:
1451:
1448:
1443:
1440:
1434:
1433:
1430:
1427:
1424:
1419:
1416:
1410:
1409:
1406:
1403:
1400:
1395:
1393:
1387:
1386:
1383:
1380:
1377:
1372:
1369:
1363:
1362:
1359:
1356:
1353:
1348:
1345:
1339:
1338:
1335:
1332:
1329:
1324:
1321:
1315:
1314:
1311:
1309:
1306:
1301:
1298:
1292:
1291:
1288:
1285:
1282:
1277:
1274:
1268:
1267:
1264:
1261:
1258:
1253:
1250:
1244:
1243:
1240:
1237:
1234:
1229:
1226:
1220:
1219:
1216:
1213:
1210:
1205:
1202:
1196:
1195:
1192:
1189:
1186:
1181:
1179:
1173:
1172:
1169:
1167:
1164:
1159:
1156:
1150:
1149:
1146:
1144:
1141:
1136:
1133:
1127:
1126:
1123:
1120:
1117:
1112:
1109:
1103:
1102:
1097:
1087:
1077:
1067:
1062:
1049:
1048:
1045:
1042:
1039:
1034:
1031:
1025:
1024:
1021:
1018:
1015:
1010:
1007:
1001:
1000:
997:
995:
992:
987:
984:
978:
977:
974:
971:
968:
963:
960:
954:
953:
950:
948:
945:
940:
937:
931:
930:
927:
924:
921:
916:
913:
907:
906:
903:
900:
897:
892:
889:
883:
882:
879:
876:
873:
868:
865:
859:
858:
856:
854:
851:
846:
843:
837:
836:
833:
830:
827:
822:
819:
813:
812:
809:
806:
803:
798:
795:
789:
788:
785:
782:
779:
774:
771:
765:
764:
761:
758:
755:
750:
747:
741:
740:
737:
735:
732:
727:
724:
718:
717:
714:
712:
709:
704:
701:
695:
694:
691:
689:
686:
681:
678:
672:
671:
668:
666:
663:
658:
655:
649:
648:
645:
642:
639:
634:
631:
625:
624:
621:
619:
616:
611:
608:
602:
601:
598:
596:
593:
588:
585:
579:
578:
575:
573:
570:
565:
562:
556:
555:
553:
550:
547:
542:
540:
534:
533:
530:
527:
524:
519:
517:
511:
510:
507:
504:
501:
496:
493:
487:
486:
483:
481:
478:
473:
470:
464:
463:
460:
458:
455:
450:
447:
441:
440:
437:
434:
431:
426:
423:
416:
415:
412:
410:
407:
402:
400:
394:
393:
390:
388:
385:
380:
377:
371:
370:
365:
355:
345:
335:
330:
303:
300:
267:dwarf galaxies
229:
226:
224:
221:
152:constellations
138:
137:
126:
125:
121:
120:
117:
113:
112:
107:
103:
102:
99:
93:
92:
87:
81:
80:
67:
60:
59:
51:
50:
43:
35:
34:
26:
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259:spectral line
256:
252:
248:
247:hydrogen line
244:
234:
220:
218:
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198:
196:
195:spiral galaxy
192:
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176:
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156:
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149:
146:is a complex
145:
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71:
68:
65:
64:Constellation
61:
57:
52:
47:
41:
36:
31:
23:
19:
2345:cite journal
2302:
2298:
2291:
2256:
2252:
2245:
2200:
2196:
2189:Spekkens, K.
2182:
2169:
2156:
2113:
2109:
2099:
2075:(1): 21–31.
2072:
2068:
2028:
2024:
2014:
1971:
1967:
1961:
1943:cite journal
1900:
1894:
1887:
1873:cite journal
1830:
1826:
1819:
1776:
1772:
1766:
1754:. Retrieved
1750:
1741:
1724:
1720:
1714:
1697:
1693:
1661:
1609:
1605:
1573:. Retrieved
1569:
1512:
1506:
1461:
1054:
322:
305:
289:
239:
210:
205:
201:
199:
179:radio galaxy
143:
141:
1756:13 February
1700:: 211–233.
1476:ESO 381-018
1464:ESO 219-010
1296:LEDA 166164
1272:LEDA 166163
1107:AM 1321-304
722:LEDA 166179
699:LEDA 166175
676:LEDA 166172
653:LEDA 166167
629:LEDA 166152
422:(NGC 5128)
420:Centaurus A
312:Centaurus A
302:Member list
296:Local Group
285:Centaurus A
253:and in the
217:Local Group
177:, a nearby
175:Centaurus A
110:Centaurus A
97:Declination
46:Centaurus A
2365:Categories
2266:2011.04990
2210:1512.05366
1575:2006-11-22
1498:References
1446:13 36 31.1
1422:13 37 20.0
1398:13 35 08.1
1375:13 41 36.7
1351:13 39 55.9
1327:13 37 00.9
1304:13 22 56.2
1280:13 21 08.2
1256:13 36 35.5
1232:13 40 18.4
1208:13 26 44.4
1184:13 36 56.1
1162:13 46 40.4
1139:13 21 32.4
1115:13 24 36.2
1037:13 57 01.4
1013:13 45 00.5
990:13 42 05.6
966:13 27 37.4
943:13 22 02.0
919:13 21 47.4
895:13 13 09.1
878:1853 ± 32
871:13 10 32.9
849:13 03 33.6
825:13 37 39.0
801:13 33 44.0
777:13 21 57.6
753:13 05 27.5
730:13 48 46.4
707:13 46 16.8
684:13 43 36.0
661:13 27 27.8
637:13 05 02.1
614:13 41 38.1
591:13 22 12.8
568:12 44 21.5
545:13 51 12.0
522:13 48 47.0
499:13 37 25.3
476:13 46 00.8
453:13 12 45.2
429:13 25 27.6
405:13 48 09.1
383:13 11 13.8
316:Messier 83
191:Messier 83
2283:226289648
2237:119251158
2203:(1): 19.
1935:119373447
1865:118921426
1811:119495338
1727:: 47–90.
1644:119385141
1492:NGC 5011C
1484:PGC 43048
1472:PGC 51659
1468:PGC 39032
1414:PGC 48111
1391:PGC 47885
1239:674 ± 53
1215:274 ± 65
1044:561 ± 32
1029:PGC 49615
1005:PGC 48738
982:PGC 48515
958:PGC 47171
935:PGC 46680
911:PGC 46663
902:784 ± 31
887:PGC 45916
863:PGC 45717
841:PGC 45104
808:571 ± 10
261:with the
206:M83 Group
159:Centaurus
74:Centaurus
2337:15027152
2148:14755909
2006:17127678
1779:: 1313.
1480:NGC 5408
1453:573 ± 1
1438:UGCA 365
1429:587 ± 3
1382:478 ± 3
1367:NGC 5264
1358:407 ± 3
1343:NGC 5253
1334:513 ± 2
1323:SAB(s)c
1287:571 ± 3
1228:IBm pec
1122:487 ± 1
1090:Redshift
1020:545 ± 2
973:516 ± 3
832:361 ± 4
817:NGC 5237
793:NGC 5206
784:468 ± 2
769:NGC 5102
760:563 ± 3
749:SB(s)cd
745:NGC 4945
657:dI/dSph
644:617 ± 4
552:529 ± 6
529:581 ± 8
506:492 ± 4
436:547 ± 5
358:Redshift
255:hydrogen
204:and the
2317:Bibcode
2259:: A92.
2215:Bibcode
2128:Bibcode
2077:Bibcode
2033:Bibcode
1986:Bibcode
1915:Bibcode
1845:Bibcode
1791:Bibcode
1729:Bibcode
1702:Bibcode
1624:Bibcode
1371:IB(s)m
1347:Im pec
1224:IC 4316
1200:IC 4247
1033:dS0/Im
1009:IB(s)m
867:I0 pec
797:SB(r)0
425:S0 pec
257:-alpha
223:Members
150:in the
2335:
2281:
2235:
2146:
2004:
1933:
1863:
1809:
1672:
1642:
1519:
1482:, and
1470:, and
1405:13848
1248:KK 208
1135:dE/Im
606:KKs 57
583:KKs 55
564:E/Sph
560:KKs 51
276:HIDEEP
271:HIPASS
185:(4.56
169:(3.66
161:, and
90:13 20
76:, and
2333:S2CID
2307:arXiv
2279:S2CID
2261:arXiv
2233:S2CID
2205:arXiv
2144:S2CID
2118:arXiv
2002:S2CID
1976:arXiv
1931:S2CID
1905:arXiv
1861:S2CID
1835:arXiv
1807:S2CID
1781:arXiv
1640:S2CID
1614:arXiv
1456:15.4
1432:15.0
1408:15.8
1385:12.6
1361:10.9
1313:17.6
1300:dSph
1290:17.1
1266:14.3
1242:15.0
1218:14.4
1194:17.3
1158:dSph
1148:17.6
1125:16.7
1084:J2000
1074:J2000
1061:Name
1047:14.8
1023:14.0
999:17.6
976:12.9
962:IABm
952:16.6
929:16.1
905:14.1
881:13.3
845:IABm
835:13.2
811:11.6
787:10.4
726:dSph
716:19.2
703:dSph
693:18.5
680:dSph
647:16.3
623:18.1
600:18.5
577:16.7
532:16.9
509:16.5
485:17.1
462:19.3
449:dSph
414:17.5
398:Cen N
392:17.3
375:Cen 7
352:J2000
342:J2000
329:Name
163:Virgo
155:Hydra
78:Virgo
70:Hydra
56:Epoch
2351:link
1953:link
1949:link
1879:link
1758:2013
1670:ISBN
1517:ISBN
1337:8.2
1263:381
1191:591
1171:19.
1111:dIm
1092:(km/
1080:Dec.
1070:R.A.
1065:Type
926:741
915:IBm
773:SA0
763:9.3
610:Sph
587:Sph
439:7.8
379:Sph
360:(km/
348:Dec.
338:R.A.
333:Type
314:and
290:The
142:The
44:The
2325:doi
2303:374
2271:doi
2257:645
2223:doi
2201:823
2136:doi
2114:133
2085:doi
2073:385
2041:doi
2029:119
1994:doi
1972:119
1923:doi
1901:346
1853:doi
1831:524
1799:doi
1777:114
1725:100
1632:doi
1610:129
1442:Im
1418:Im
1319:M83
1276:dI
1252:dI
986:dE
939:Im
891:dE
821:I0
739:18
670:18
633:dI
495:Im
472:dE
187:Mpc
183:Mly
171:Mpc
167:Mly
136:344
134:LGG
130:NGC
66:(s)
20:or
2367::
2347:}}
2343:{{
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