976:; Cushing, Michael C.; Gelino, Christopher R.; Griffith, Roger L.; Skrutskie, Michael F.; Marsh, Kenneth A.; Wright, Edward L.; Mainzer, Amy K.; Eisenhardt, Peter R.; McLean, Ian S.; Thompson, Maggie A.; Bauer, James M.; Benford, Dominic J.; Bridge, Carrie R.; Lake, Sean E.; Petty, Sara M.; Stanford, Spencer Adam; Tsai, Chao-Wei; Bailey, Vanessa; Beichman, Charles A.; Bloom, Joshua S.; Bochanski, John J.; Burgasser, Adam J.; Capak, Peter L.; Cruz, Kelle L.; Hinz, Philip M.; Kartaltepe, Jeyhan S.; Knox, Russell P.; Manohar, Swarnima; Masters, Daniel; Morales-Calderon, Maria; Prato, Lisa A.; Rodigas, Timothy J.; Salvato, Mara; Schurr, Steven D.; Scoville, Nicholas Z.; Simcoe, Robert A.; Stapelfeldt, Karl R.; Stern, Daniel; Stock, Nathan D.; Vacca, William D. (2011). "The First Hundred Brown Dwarfs Discovered by the Wide-field Infrared Survey Explorer (WISE)".
1124:
Mainzer, A.; Cushing, Michael C.; Skrutskie, M.; Gelino, C. R.; Kirkpatrick, J. Davy; Jarrett, T.; Masci, F.; Marley, Mark S.; Saumon, D.; Wright, E.; Beaton, R.; Dietrich, M.; Eisenhardt, P.; Garnavich, P.; Kuhn, O.; Leisawitz, D.; Marsh, K.; McLean, I.; Padgett, D.; Rueff, K. (2011). "The First
634:
WISE 1841+7000 was discovered in 2011 from data, collected by Wide-field
Infrared Survey Explorer (WISE) Earth-orbiting satellite — NASA infrared-wavelength 40 cm (16 in) space telescope, which mission lasted from December 2009 to February 2011. WISE 1841+7000A has two discovery papers:
912:
These 98 brown dwarf systems are only among first, not all brown dwarf systems, discovered from data, collected by WISE: six discoveries were published earlier (however, also listed in
Kirkpatrick et al. (2011)) in Mainzer et al. (2011) and Burgasser et al. (2011), and the other discoveries were
1180:
Burgasser, Adam J.; Cushing, Michael C.; Kirkpatrick, J. Davy; Gelino, Christopher R.; Griffith, Roger L.; Looper, Dagny L.; Tinney, Christopher; Simcoe, Robert A.; Bochanski, John J.; Skrutskie, Michael F.; Mainzer, A.; Thompson, Maggie A.; Marsh, Kenneth A.; Bauer, James M.; Wright, Edward L.
36:
1068:
Gelino, Christopher R.; Kirkpatrick, J. Davy; Cushing, Michael C.; Eisenhardt, Peter R.; Griffith, Roger L.; Mainzer, Amanda K.; Marsh, Kenneth A.; Skrutskie, Michael F.; Wright, Edward L. (2011). "WISE Brown Dwarf
Binaries: The Discovery of a T5+T5 and a T8.5+T9 System".
922:
Presented in Gelino et al. (2011), but this is not mentioned in
Kirkpatrick et al. (2011) and Kirkpatrick et al. (2012) — according to these two articles, the only discovery paper of WISE 0750+2725 is Kirkpatrick et al.
662:; seven of these nine brown dwarfs were also newfound, including WISE 1841+7000. These observations had indicated that two of these nine brown dwarfs, including WISE 1841+7000, are binary.
711:
of WISE 1841+7000 is not yet measured. Therefore, there are only distance estimates of this object, obtained by indirect — spectrofotometric — means (see table).
978:
47:
570:
565:
65:
1256:
1251:
879:
873:
867:
857:
851:
839:
824:
845:
1183:
1127:
200:
162:
128:
1181:(2011). "Fire Spectroscopy of Five Late-type T Dwarfs Discovered with the Wide-field Infrared Survey Explorer".
591:
1071:
708:
1261:
1246:
1241:
659:
615:
298:
281:
249:
232:
179:
145:
80:
1202:
1146:
1090:
997:
543:
357:
61:
973:
664:
1218:
1192:
1162:
1136:
1106:
1080:
1013:
987:
293:
276:
244:
227:
191:
174:
157:
140:
123:
35:
550:
501:
58:
1210:
1154:
1098:
1005:
697:
690:
655:
648:
516:
693:
651:
88:
1206:
1150:
1094:
1001:
726:
611:
557:
531:
523:
507:
409:
345:
333:
1214:
1235:
1158:
1102:
1009:
674:
322:
266:
217:
75:
1222:
1166:
1110:
1017:
467:
460:
442:
435:
670:
607:
101:
1125:
Ultra-cool Brown Dwarf
Discovered by the Wide-field Infrared Survey Explorer".
738:
619:
364:
310:
17:
626:. It is notable for being one of the first known binary brown dwarf systems.
732:
585:
369:
992:
1197:
1141:
1085:
623:
381:
68:
417:
349:
337:
700:. It was presented in the same article as the component A.
677:
M, L, T and Y, among which also was WISE 1841+7000.
796:Non-trigonometric distance estimates are marked in
292:
275:
265:
260:
243:
226:
216:
211:
190:
173:
156:
139:
122:
117:
110:
968:
966:
964:
962:
960:
958:
956:
954:
952:
950:
948:
946:
944:
942:
940:
938:
813:The other eight objects, checked for binarity by
685:Component B of the system was discovered in 2011
827:(T8.5 + T9.5, component A discovered before by
647:examined for binarity nine brown dwarfs using
1063:
1061:
1059:
1057:
1055:
1053:
1051:
1049:
1047:
8:
1045:
1043:
1041:
1039:
1037:
1035:
1033:
1031:
1029:
1027:
669:presented discovery of 98 new found by WISE
64:55590.80
106:70° 00′ 38.54″
1196:
1140:
1084:
991:
899:
897:
718:
934:
893:
329:
26:
7:
979:The Astrophysical Journal Supplement
903:For an assumed system age of 1 Gyr.
341:
614:T5 + T5, located in constellation
25:
800:. The best estimate is marked in
715:WISE 1841+7000 distance estimates
34:
602:(designation is abbreviated to
1:
1215:10.1088/0004-637X/735/2/116
673:systems with components of
28:WISEPA J184124.74+700038.0
1278:
1159:10.1088/0004-637X/726/1/30
1103:10.1088/0004-6256/142/2/57
1010:10.1088/0067-0049/197/2/19
860:(T8, discovered before by
600:WISEPA J184124.74+700038.0
1184:The Astrophysical Journal
1128:The Astrophysical Journal
771:Kirkpatrick et al. (2011)
641:Kirkpatrick et al. (2011)
578:
563:
556:
478:
453:
428:
423:
380:
376:
316:
309:
55:
32:
1072:The Astronomical Journal
606:) is a binary system of
480:Position (relative to A)
862:Burgasser et al. (2011)
774:(not assuming binarity)
709:Trigonometric parallax
681:Discovery of companion
1257:Draco (constellation)
829:Mainzer et al. (2011)
618:at approximately 131
332: -104 ± 25
974:Kirkpatrick, J. Davy
836:binarity not found:
815:Gelino et al. (2011)
748:Gelino et al. (2011)
637:Gelino et al. (2011)
544:Projected separation
502:Epoch of observation
344: 527 ± 28
1252:T-type brown dwarfs
1207:2011ApJ...735..116B
1151:2011ApJ...726...30M
1095:2011AJ....142...57G
1002:2011ApJS..197...19K
696:system (LGS-AO) on
654:system (LGS-AO) on
579:Database references
568:J184124.74+700038.0
29:
558:Other designations
294:Apparent magnitude
277:Apparent magnitude
245:Apparent magnitude
228:Apparent magnitude
192:Apparent magnitude
175:Apparent magnitude
158:Apparent magnitude
141:Apparent magnitude
124:Apparent magnitude
27:
805:
793:
792:
775:
698:Keck II telescope
656:Keck II telescope
597:
596:
368:(40.2 ± 4.9
302:
285:
253:
236:
204:
183:
166:
149:
132:
16:(Redirected from
1269:
1227:
1226:
1200:
1177:
1171:
1170:
1144:
1121:
1115:
1114:
1088:
1065:
1022:
1021:
995:
970:
924:
920:
914:
913:published later.
910:
904:
901:
842:(T8.5, newfound)
821:binarity found:
795:
773:
719:
691:Laser Guide Star
649:Laser Guide Star
612:spectral classes
517:Angular distance
363:131.1 ± 16
343:
331:
296:
279:
247:
230:
194:
177:
160:
143:
126:
96:
91:
56:Observation data
38:
30:
21:
1277:
1276:
1272:
1271:
1270:
1268:
1267:
1266:
1232:
1231:
1230:
1179:
1178:
1174:
1123:
1122:
1118:
1067:
1066:
1025:
972:
971:
936:
932:
927:
921:
917:
911:
907:
902:
895:
891:
811:
772:
706:
694:Adaptive Optics
683:
652:Adaptive Optics
632:
574:
569:
473:
448:
367:
340:
301:filter system))
284:filter system))
252:filter system))
235:filter system))
203:filter system))
198:
182:filter system))
165:filter system))
148:filter system))
131:filter system))
113:
112:Characteristics
94:
89:Right ascension
87:
57:
51:
41:
39:
23:
22:
15:
12:
11:
5:
1275:
1273:
1265:
1264:
1259:
1254:
1249:
1244:
1234:
1233:
1229:
1228:
1172:
1116:
1023:
933:
931:
928:
926:
925:
915:
905:
892:
890:
887:
886:
885:
884:
883:
882:(T9, newfound)
880:WISE 1741+2553
877:
876:(T8, newfound)
874:WISE 1653+4444
871:
870:(T6, newfound)
868:WISE 1627+3255
865:
858:WISE 1617+1807
855:
854:(T9, newfound)
852:WISE 1614+1739
849:
848:(T8, newfound)
846:WISE 1322-2340
843:
840:WISE 0750+2725
834:
833:
832:
825:WISE 0458+6434
810:
807:
791:
790:
788:
783:
778:
776:
768:
767:
765:
758:
751:
749:
745:
744:
741:
735:
729:
723:
705:
702:
682:
679:
675:spectral types
631:
628:
604:WISE 1841+7000
595:
594:
589:
581:
580:
576:
575:
564:
561:
560:
554:
553:
547:
539:
538:
535:
532:Position angle
527:
526:
520:
512:
511:
505:
497:
496:
493:
487:
486:
483:
482:
476:
475:
471:
464:
456:
455:
451:
450:
446:
439:
431:
430:
426:
425:
421:
420:
414:
405:
404:
401:
395:
394:
391:
385:
384:
378:
377:
374:
373:
361:
353:
352:
327:
318:
317:
314:
313:
307:
306:
303:
290:
289:
286:
273:
272:
269:
263:
262:
258:
257:
254:
241:
240:
237:
224:
223:
220:
214:
213:
209:
208:
205:
196:
188:
187:
184:
171:
170:
169:16.912 ± 0.082
167:
154:
153:
150:
137:
136:
135:16.800 ± 0.035
133:
120:
119:
115:
114:
111:
108:
107:
104:
98:
97:
92:
84:
83:
78:
72:
71:
53:
52:
48:legacy surveys
40:WISE 1841+7000
33:
24:
18:WISE 1841+7000
14:
13:
10:
9:
6:
4:
3:
2:
1274:
1263:
1260:
1258:
1255:
1253:
1250:
1248:
1245:
1243:
1240:
1239:
1237:
1224:
1220:
1216:
1212:
1208:
1204:
1199:
1194:
1190:
1186:
1185:
1176:
1173:
1168:
1164:
1160:
1156:
1152:
1148:
1143:
1138:
1134:
1130:
1129:
1120:
1117:
1112:
1108:
1104:
1100:
1096:
1092:
1087:
1082:
1078:
1074:
1073:
1064:
1062:
1060:
1058:
1056:
1054:
1052:
1050:
1048:
1046:
1044:
1042:
1040:
1038:
1036:
1034:
1032:
1030:
1028:
1024:
1019:
1015:
1011:
1007:
1003:
999:
994:
989:
985:
981:
980:
975:
969:
967:
965:
963:
961:
959:
957:
955:
953:
951:
949:
947:
945:
943:
941:
939:
935:
929:
919:
916:
909:
906:
900:
898:
894:
888:
881:
878:
875:
872:
869:
866:
863:
859:
856:
853:
850:
847:
844:
841:
838:
837:
835:
830:
826:
823:
822:
820:
819:
818:
816:
808:
806:
803:
799:
789:
787:
784:
782:
779:
777:
770:
769:
766:
764:
763:
759:
757:
756:
752:
750:
747:
746:
742:
740:
736:
734:
730:
728:
724:
721:
720:
717:
716:
712:
710:
703:
701:
699:
695:
692:
688:
687:Gelino et al.
680:
678:
676:
672:
668:
666:
661:
657:
653:
650:
646:
645:Gelino et al.
642:
638:
629:
627:
625:
621:
617:
613:
609:
605:
601:
593:
590:
588:
587:
583:
582:
577:
572:
567:
562:
559:
555:
552:
548:
546:
545:
541:
540:
537:82 ± 9°
536:
534:
533:
529:
528:
525:
521:
519:
518:
514:
513:
509:
506:
504:
503:
499:
498:
494:
492:
489:
488:
485:
484:
481:
477:
474:
470:
465:
463:
462:
458:
457:
452:
449:
445:
440:
438:
437:
433:
432:
427:
422:
419:
415:
413:
411:
407:
406:
402:
400:
397:
396:
392:
390:
387:
386:
383:
379:
375:
371:
366:
362:
360:
359:
355:
354:
351:
347:
339:
335:
328:
326:
324:
323:Proper motion
320:
319:
315:
312:
308:
304:
300:
295:
291:
287:
283:
278:
274:
270:
268:
267:Spectral type
264:
259:
255:
251:
246:
242:
238:
234:
229:
225:
221:
219:
218:Spectral type
215:
210:
206:
202:
193:
189:
185:
181:
176:
172:
168:
164:
159:
155:
151:
147:
142:
138:
134:
130:
125:
121:
116:
109:
105:
103:
100:
99:
93:
90:
86:
85:
82:
79:
77:
76:Constellation
74:
73:
70:
67:
63:
60:
54:
50:
49:
44:
37:
31:
19:
1262:WISE objects
1247:Brown dwarfs
1242:Binary stars
1188:
1182:
1175:
1132:
1126:
1119:
1076:
1070:
983:
977:
918:
908:
861:
828:
817:on Keck II:
814:
812:
801:
797:
794:
785:
780:
761:
760:
754:
753:
714:
713:
707:
686:
684:
663:
644:
640:
636:
633:
608:brown dwarfs
603:
599:
598:
584:
542:
530:
515:
500:
490:
479:
468:
459:
443:
434:
408:
398:
388:
356:
321:
305:17.75 ± 0.10
288:17.57 ± 0.13
256:17.73 ± 0.10
239:17.24 ± 0.10
186:16.99 ± 0.04
152:16.64 ± 0.03
118:Whole system
46:
42:
993:1108.4677v1
671:brown dwarf
665:Kirkpatrick
620:light-years
573:J1841+7000
454:Component B
429:Component A
261:Component B
212:Component A
102:Declination
95:18 41 24.75
1236:Categories
1191:(2): 116.
930:References
762:131.1 ± 16
755:40.2 ± 4.9
737:Distance,
731:Distance,
725:Parallax,
549:2.8 ± 0.7
510:2010 Jul 1
311:Astrometry
207:>15.626
1198:1104.2537
1142:1011.2279
1135:(1): 30.
1086:1106.3142
1079:(2): 57.
986:(2): 19.
660:Mauna Kea
630:Discovery
491:Component
466:≈60
441:≈60
399:Companion
1223:19003973
1167:20700414
1111:51345460
1018:16850733
809:See also
704:Distance
522:70 ± 14
358:Distance
1203:Bibcode
1147:Bibcode
1091:Bibcode
998:Bibcode
923:(2011).
424:Details
389:Primary
66:Equinox
1221:
1165:
1109:
1016:
798:italic
722:Source
667:et al.
586:SIMBAD
566:WISEPA
410:Period
43:Credit
1219:S2CID
1193:arXiv
1163:S2CID
1137:arXiv
1107:S2CID
1081:arXiv
1014:S2CID
988:arXiv
889:Notes
786:~73,1
781:~22,4
743:Ref.
689:with
624:Earth
622:from
616:Draco
382:Orbit
342:Dec.:
201:2MASS
163:2MASS
129:2MASS
81:Draco
69:J2000
59:Epoch
802:bold
639:and
592:data
571:WISE
461:Mass
436:Mass
416:~11
297:(H (
280:(J (
248:(H (
231:(J (
178:(H (
161:(H (
144:(J (
127:(J (
1211:doi
1189:735
1155:doi
1133:726
1099:doi
1077:142
1006:doi
984:197
727:mas
658:on
610:of
524:mas
472:Jup
447:Jup
412:(P)
346:mas
334:mas
330:RA:
325:(μ)
299:MKO
282:MKO
250:MKO
233:MKO
180:MKO
146:MKO
62:MJD
1238::
1217:.
1209:.
1201:.
1187:.
1161:.
1153:.
1145:.
1131:.
1105:.
1097:.
1089:.
1075:.
1026:^
1012:.
1004:.
996:.
982:.
937:^
896:^
739:ly
733:pc
643:.
551:AU
508:UT
418:yr
370:pc
365:ly
350:yr
338:yr
271:T5
222:T5
195:(K
45::
1225:.
1213::
1205::
1195::
1169:.
1157::
1149::
1139::
1113:.
1101::
1093::
1083::
1020:.
1008::
1000::
990::
864:)
831:)
804:.
495:B
469:M
444:M
403:B
393:A
372:)
348:/
336:/
199:(
197:S
20:)
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