1270:
32:
762:
Skrutskie, M. F.; Cutri, R. M.; Stiening, R.; Weinberg, M. D.; Schneider, S.; Carpenter, J. M.; Beichman, C.; Capps, R.; Chester, T.; Elias, J.; Huchra, J.; Liebert, J.; Lonsdale, C.; Monet, D. G.; Price, S.; Seitzer, P.; Jarrett, T.; Kirkpatrick, J. D.; Gizis, J. E.; Howard, E.; Evans, T.; Fowler,
1312:
376:
in
November 1835. A month later, he observed NGC 1570 again and mistakenly called it NGC 1571 due to imprecise coordinates. NGC 1570 is part of a small
37:
330:
172:
763:
J.; Fullmer, L.; Hurt, R.; Light, R.; Kopan, E. L.; Marsh, K. A.; McCallon, H. L.; Tam, R.; Van Dyk, S.; Wheelock, S. (February 2006).
256:
479:
Paturel, G.; Dubois, P.; Petit, C.; Woelfel, F. (2002). "Comparison LEDA/SIMBAD octobre 2002. Catalogue to be published in 2003".
928:
509:
Crook, Aidan C.; Huchra, John P.; Martimbeau, Nathalie; Masters, Karen L.; Jarrett, Tom; Macri, Lucas M. (February 2007).
1297:
1292:
263:
889:
NGC 2000.0: The
Complete New General Catalogue and Index Catalogues of Nebulae and Star Clusters by J. L. E. Dreyer
1020:
455:
948:
1106:
937:
121:
1317:
1199:
1043:
292:
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22:
1307:
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843:
776:
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651:
610:
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532:
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427:
861:
833:
794:
736:
708:
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641:
550:
522:
445:
417:
153:
967:
869:
802:
744:
677:
558:
373:
338:
334:
50:
369:'s. NGC 1570 is said to be round in shape, making it more likely to be an elliptical galaxy.
851:
847:
784:
726:
722:
659:
655:
540:
435:
431:
322:
220:
113:
1302:
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914:
316:
102:
70:
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614:
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536:
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143:
1286:
449:
354:
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235:
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58:
31:
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1005:
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139:
664:
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731:
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995:
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82:
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342:
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208:
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127:
873:
865:
806:
798:
748:
740:
681:
673:
562:
554:
1243:
1158:
358:
296:
822:"Star formation history of early-type galaxies in low density environments"
906:
856:
821:
1222:
1217:
1212:
1140:
1135:
1119:
1114:
1096:
1091:
1086:
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1033:
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1010:
838:
713:
527:
300:
92:
990:
47:
1190:
459:
288:
281:
212:
131:
63:
697:"The gas content of peculiar galaxies: Strongly interacting systems"
789:
764:
545:
510:
422:
820:
Longhetti, M.; Rampazzo, R.; Bressan, A.; Chiosi, C. (June 1998).
646:
958:
362:
346:
182:
910:
511:"Groups of Galaxies in the Two Micron All Sky Redshift Survey"
366:
350:
406:
Data
Release 3. Summary of the content and survey properties"
581:
The surface photometry catalogue of the ESO-Uppsala galaxies
695:
Casasola, V.; Bettoni, D.; Galletta, G. (16 July 2004).
400:
Vallenari, A.; et al. (Gaia collaboration) (2023).
1231:
1198:
1189:
1157:
1128:
1105:
1042:
1019:
966:
957:
630:"The mass function of nearby black hole candidates"
303:of z = 0.014760, the object is estimated to be 198
242:
219:
203:
181:
171:
166:
152:
138:
120:
101:
91:
81:
69:
57:
45:
21:
295:of 13.2, making it visible through a medium sized
628:Caramete, L. I.; Biermann, P. L. (October 2010).
315:. It appears to be receding with a heliocentric
600:
598:
579:Lauberts, Andris; Valentijn, Edwin A. (1989).
574:
572:
922:
474:
472:
470:
468:
8:
826:Astronomy and Astrophysics Supplement Series
380:called LDC 302. It is the brightest member.
365:abundance of the galaxy is 135% that of the
337:. It has also been catalogued as a peculiar
87:−43° 37′ 46.4517″
504:
502:
500:
498:
1195:
1154:
963:
929:
915:
907:
30:
855:
837:
788:
730:
712:
663:
645:
544:
526:
439:
421:
395:
393:
224:
765:"The Two Micron All Sky Survey (2MASS)"
389:
607:ESO/Uppsala survey of the ESO(B) atlas
18:
16:Galaxy in the constellation of Caelum
7:
1313:Principal Galaxies Catalogue objects
372:The galaxy was first discovered by
331:galaxy morphological classification
157:
14:
1269:
1268:
456:Gaia DR3 record for this source
333:of S0, indicating that it is a
1:
353:. It is estimated to be 8.9
103:Heliocentric radial velocity
665:10.1051/0004-6361/200913146
441:10.1051/0004-6361/202243940
1334:
887:Sinnott, Roger W. (1988).
732:10.1051/0004-6361:20040283
701:Astronomy and Astrophysics
634:Astronomy and Astrophysics
410:Astronomy and Astrophysics
1266:
1153:
944:
515:The Astrophysical Journal
247:
29:
769:The Astronomical Journal
284:located in the southern
949:List of stars in Caelum
938:Constellation of Caelum
848:1998A&AS..130..251L
723:2004A&A...422..941C
656:2010A&A...521A..55C
432:2023A&A...674A...1G
291:, the chisel. It has a
357:old, younger than the
349:297 times that of the
191:149 (black hole)
605:Lauberts, A. (1982).
276:, mistakenly called
1298:Elliptical galaxies
1293:Lenticular galaxies
897:1988cngc.book.....S
857:10.1051/aas:1998410
781:2006AJ....131.1163S
615:1982euse.book.....L
589:1989spce.book.....L
537:2007ApJ...655..790C
489:2002LEDA.........0P
305:million light years
243:Other designations
154:Apparent magnitude
46:Observation data (
40:image of NGC 1570.
1280:
1279:
1262:
1261:
1185:
1184:
1149:
1148:
374:Sir John Herschel
339:elliptical galaxy
335:lenticular galaxy
271:
270:
226:
159:
1325:
1272:
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1196:
1155:
964:
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900:
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878:
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841:
839:astro-ph/9910032
817:
811:
810:
792:
775:(2): 1163–1183.
759:
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734:
716:
714:astro-ph/0405112
692:
686:
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667:
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625:
619:
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528:astro-ph/0610732
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311:) away from the
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329:NGC 1570 has a
320:
317:radial velocity
262:
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167:Characteristics
109:
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75:
71:Right ascension
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832:(2): 251–265.
812:
790:10.1086/498708
754:
707:(3): 941–950.
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620:
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568:
546:10.1086/510201
521:(2): 790–813.
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361:. The average
341:. The central
293:blue magnitude
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76:04 22 08.93282
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38:legacy surveys
35:
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355:billion years
352:
348:
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318:
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306:
302:
299:. Based on a
298:
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287:
286:constellation
283:
280:, is a faint
279:
275:
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258:
251:
246:
241:
237:
233:
228:
222:
221:Apparent size
218:
214:
211:(33,113
210:
207:108,000
206:
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68:
65:
62:
60:
59:Constellation
56:
52:
49:
44:
39:
33:
28:
24:
20:
1318:LEDA objects
1249:PKS 0438-436
1207:
888:
882:
829:
825:
815:
772:
768:
757:
704:
700:
690:
637:
633:
623:
606:
580:
518:
514:
480:
413:
409:
403:
378:galaxy group
371:
328:
277:
273:
272:
1308:NGC objects
1254:PKS 0451-28
1239:HE0450-2958
321:4,392
313:Local Group
309:megaparsecs
130:(60.9
83:Declination
1287:Categories
1177:WASP-159 b
1172:RR Caeli b
1167:HD 30669 b
1159:Exoplanets
423:2208.00211
384:References
343:black hole
1244:PGC 16389
874:0365-0138
866:1286-4846
807:0004-6256
799:1538-3881
749:0004-6361
741:1432-0746
682:0004-6361
674:1432-0746
647:0908.2764
563:0004-637X
555:1538-4357
450:244398875
359:Milky Way
297:telescope
126:199
1274:Category
1191:Galaxies
1141:LHS 1678
1136:WASP-159
1021:Variable
301:redshift
278:NGC 1571
274:NGC 1570
197:☉
122:Distance
112:84
97:0.014760
93:Redshift
893:Bibcode
844:Bibcode
777:Bibcode
719:Bibcode
652:Bibcode
640:: A55.
611:Bibcode
585:Bibcode
533:Bibcode
485:Bibcode
428:Bibcode
234:× 0.809
148:LDC 302
144:cluster
48:J2000.0
1303:Caelum
872:
864:
805:
797:
747:
739:
680:
672:
561:
553:
460:VizieR
448:
416:: A1.
345:has a
307:(60.9
289:Caelum
282:galaxy
223:
156:
64:Caelum
1232:Other
1129:Other
1120:30669
1115:29559
968:Bayer
959:Stars
862:eISSN
834:arXiv
795:eISSN
737:eISSN
709:arXiv
670:eISSN
642:arXiv
551:eISSN
523:arXiv
483:: 0.
454:
446:S2CID
418:arXiv
266:14971
259:14971
230:1.037
162:13.22
140:Group
108:4,392
51:epoch
1223:1701
1218:1616
1213:1571
1208:1570
1097:1651
1092:1635
1087:1631
1082:1584
1077:1559
1072:1526
1067:1509
1062:1433
1057:1418
1052:1404
870:ISSN
803:ISSN
745:ISSN
678:ISSN
559:ISSN
481:LEDA
404:Gaia
363:iron
347:mass
323:km/s
257:LEDA
252:1571
204:Size
183:Mass
173:Type
114:km/s
25:1570
1200:NGC
852:doi
830:130
785:doi
773:131
727:doi
705:422
660:doi
638:521
541:doi
519:655
458:at
436:doi
414:674
367:Sun
351:Sun
319:of
264:PGC
250:NGC
225:(V)
187:297
158:(B)
142:or
132:Mpc
128:Mly
23:NGC
1289::
1107:HD
1044:HR
1034:RV
1029:RR
891:.
868:.
860:.
850:.
842:.
828:.
824:.
801:.
793:.
783:.
771:.
767:.
743:.
735:.
725:.
717:.
703:.
699:.
676:.
668:.
658:.
650:.
636:.
632:.
609:.
597:^
583:.
571:^
557:.
549:.
539:.
531:.
517:.
513:.
497:^
467:^
444:.
434:.
426:.
412:.
408:.
392:^
326:.
261:,
254:,
213:pc
209:ly
177:S0
36:A
1011:ν
1006:λ
1001:ζ
996:δ
991:γ
986:γ
981:β
976:α
930:e
923:t
916:v
899:.
895::
876:.
854::
846::
836::
809:.
787::
779::
751:.
729::
721::
711::
684:.
662::
654::
644::
617:.
613::
591:.
587::
565:.
543::
535::
525::
491:.
487::
462:.
452:.
438::
430::
420::
402:"
236:′
232:′
215:)
194:M
189:±
134:)
110:±
53:)
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