827:; 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)".
1763:
888:; Gelino, Christopher R.; Cushing, Michael C.; Mace, Gregory N.; Griffith, Roger L.; Skrutskie, Michael F.; Marsh, Kenneth A.; Wright, Edward L.; Eisenhardt, Peter R.; McLean, Ian S.; Mainzer, Amy K.; Burgasser, Adam J.; Tinney, Chris G.; Parker, Stephen; Salter, Graeme (2012). "Further Defining Spectral Type "Y" and Exploring the Low-mass End of the Field Brown Dwarf Mass Function".
1030:
Cushing, Michael C.; Kirkpatrick, J. Davy; Gelino, Christopher R.; Griffith, Roger L.; Skrutskie, Michael F.; Mainzer, A.; Marsh, Kenneth A.; Beichman, Charles A.; Burgasser, Adam J.; Prato, Lisa A.; Simcoe, Robert A.; Marley, Mark S.; Saumon, D.; Freedman, Richard S.; Eisenhardt, Peter R.; Wright,
773:
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
495:
WISE 2056+1459 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 2056+1459 has two discovery papers:
1188:
Marsh, Kenneth A.; Wright, Edward L.; Kirkpatrick, J. Davy; Gelino, Christopher R.; Cushing, Michael C.; Griffith, Roger L.; Skrutskie, Michael F.; Eisenhardt, Peter R. (2013). "Parallaxes and Proper
Motions of Ultracool Brown Dwarfs of Spectral Types Y and Late T".
529:
presented discovery of seven brown dwarfs — one of T9.5 type, and six of Y-type — first members of the Y spectral class, ever discovered and spectroscopically confirmed, including "archetypal member" of the Y spectral class
710:
700:
1800:
370:
962:
627:
GMOS. The researchers used the archived spectrum from
Cushing et al. and the new spectrum in this work. The cloudy model included cloud decks of
39:
829:
1259:
426:
421:
416:
411:
50:
635:
condensates. The model did fit the spectra well except for some parts due to the model not including the atmospheric mixing of
68:
1284:
1143:"James Webb Space Telescope Spectra of Cold Brown Dwarfs are Well-reproduced by Phosphine-free, Diabatic, ATMO2020++ Models"
1790:
1084:
Leggett, S. K.; Morley, Caroline V.; Marley, M. S.; Saumon, D.; Fortney, Jonathan J.; Visscher, Channon (2013-02-01).
754:
748:
736:
730:
688:. The researchers also found a medium probability (47%) of this object belonging to the Carina-Near group of stars.
1279:
742:
724:
1434:
1268:
1191:
890:
173:
135:
1086:"A Comparison of Near-infrared Photometry and Spectra for Y Dwarfs with a New Generation of Cool Cloudy Models"
447:
1031:
Edward L. (2011). "The
Discovery of Y Dwarfs using Data from the Wide-field Infrared Survey Explorer (WISE)".
1252:
656:
1547:
548:
119:
1805:
1785:
1712:
1474:
1381:
668:
378:
192:
154:
534:, and WISE 2056+1459. These seven objects are also the faintest seven of 98 brown dwarfs, presented in
1210:
1154:
1107:
1050:
981:
909:
848:
284:
64:
885:
824:
508:
1795:
1766:
1245:
1226:
1200:
1097:
1085:
1066:
1040:
999:
971:
958:"The Field Substellar Mass Function Based on the Full-sky 20 pc Census of 525 L, T, and Y Dwarfs"
925:
899:
864:
838:
624:
186:
167:
148:
129:
1303:
1172:
1123:
61:
1581:
1336:
1218:
1162:
1115:
1058:
989:
917:
856:
705:
268:
672:
531:
358:
91:
1214:
1158:
1111:
1054:
985:
913:
852:
38:
1361:
1351:
1331:
1326:
1321:
1311:
562:
467:
403:
345:
276:
256:
236:
1222:
1119:
921:
1779:
1612:
1457:
1356:
1341:
1316:
1062:
1003:
929:
860:
519:
217:
78:
1230:
868:
1645:
1622:
1346:
680:
325:
318:
1070:
1617:
1452:
1447:
1442:
1424:
1419:
1414:
1409:
1404:
1399:
1394:
1367:
664:
515:
504:, however, basically with the same authors and published nearly simultaneously.
463:
104:
1167:
1142:
994:
957:
1389:
584:
475:
291:
205:
17:
1237:
1176:
1127:
1653:
1604:
1555:
1537:
1532:
1527:
1522:
1517:
1512:
1507:
1502:
1497:
1492:
1487:
1482:
660:
471:
83:
1746:
1730:
1725:
1720:
1689:
1663:
1658:
1571:
632:
956:
Kirkpatrick, J. Davy; Gelino, Christopher R.; et al. (March 2021).
1627:
1463:
652:
644:
636:
628:
1703:
1681:
1576:
619:
573:
547:
Currently the most accurate distance estimate of WISE 2056+1459 is a
441:
392:
338:
296:
843:
976:
1205:
1102:
1045:
904:
659:. An excellent fit between spectrum and model was produced with a
479:
71:
1294:
260:
240:
1241:
676:
651:) missing in the model. WISE 2056+1459 was also observed with
716:
The other six discoveries of brown dwarfs, published in
711:
List of nearby stellar associations and moving groups
1739:
1711:
1702:
1680:
1644:
1603:
1564:
1546:
1473:
1433:
1380:
1302:
1293:
1147:
Research Notes of the
American Astronomical Society
522:
M, L, T and Y, among which also was WISE 2056+1459.
819:
817:
815:
813:
811:
809:
951:
949:
947:
945:
943:
941:
939:
880:
878:
807:
805:
803:
801:
799:
797:
795:
793:
791:
789:
675:of log g = 4.0. These values correspond to a 300
1141:Leggett, S. K.; Tremblin, Pascal (2024-01-01).
1253:
1025:
1023:
1021:
1019:
1017:
1015:
1013:
701:List of star systems within 20–25 light years
8:
514:presented discovery of 98 new found by WISE
67:55511.01
963:The Astrophysical Journal Supplement Series
1708:
1677:
1641:
1600:
1299:
1260:
1246:
1238:
109:14° 59′ 53.68″
1204:
1166:
1101:
1044:
993:
975:
903:
842:
1801:Astronomical objects discovered in 2011
785:
766:
224:
596:WISE 2056+1459 has a proper motion of
29:
612:The object's temperature estimate is
7:
830:The Astrophysical Journal Supplement
551:, published in 2021 by Kirkpatrick
244:
27:Star in the constellation Delphinus
25:
1762:
1761:
37:
623:. The object was observed with
1285:Delphinus in Chinese astronomy
566:, corresponding to a distance
1:
470:Y0, located in constellation
1223:10.1088/0004-637X/762/2/119
1120:10.1088/0004-637X/763/2/130
922:10.1088/0004-637X/753/2/156
518:systems with components of
275:140.8 ± 2.0
31:WISEPC J205628.90+145953.3
1822:
1280:List of stars in Delphinus
1269:Constellation of Delphinus
1063:10.1088/0004-637X/743/1/50
861:10.1088/0067-0049/197/2/19
604:milliarcseconds per year.
460:WISEPC J205628.90+145953.3
1759:
1676:
1640:
1599:
1275:
1192:The Astrophysical Journal
1090:The Astrophysical Journal
1033:The Astrophysical Journal
891:The Astrophysical Journal
536:Kirkpatrick et al. (2011)
498:Kirkpatrick et al. (2011)
434:
409:
402:
398:
312:
307:
303:
211:
204:
113:
58:
35:
1168:10.3847/2515-5172/ad1b61
995:10.3847/1538-4365/abd107
679:object with a mass of 5
657:Mid-Infrared Instrument
486:History of observations
187:Apparent magnitude
168:Apparent magnitude
149:Apparent magnitude
549:trigonometric parallax
474:at approximately 23.2
344:0.93 (0.86–1.01)
718:Cushing et al. (2011)
669:effective temperature
502:Cushing et al. (2011)
886:Kirkpatrick, J. Davy
825:Kirkpatrick, J. Davy
671:of 450 Kevlin and a
369:4.75 (4.5–5.0)
1791:Y-type brown dwarfs
1215:2013ApJ...762..119M
1159:2024RNAAS...8...13L
1112:2013ApJ...763..130L
1055:2011ApJ...743...50C
986:2021ApJS..253....7K
914:2012ApJ...753..156K
853:2011ApJS..197...19K
608:Physical properties
435:Database references
414:J205628.90+145953.3
32:
458:(full designation
404:Other designations
130:Apparent magnitude
120:Spectral type
30:
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1755:
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1572:HAT-P-23 (Moriah)
453:
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16:(Redirected from
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774:published later.
771:
706:List of Y-dwarfs
622:
617:
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601:
587:
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560:
390:
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324:20 (12–30)
295:(7.1 ± 0.1
290:23.2 ± 0.3
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114:Characteristics
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59:Observation data
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1582:WISE J2030+0749
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673:surface gravity
667:model using an
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1587:WISE 2056+1459
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755:WISE 1828+2650
752:
749:WISE 1738+2732
746:
743:WISE 1541-2250
740:
737:WISE 1405+5534
734:
731:WISE 0410+1502
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725:WISE 0148-7202
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532:WISE 1828+2650
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520:spectral types
492:
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468:spectral class
456:WISE 2056+1459
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1646:Star clusters
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128:
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123:
121:
118:
117:
112:
108:
106:
103:
102:
96:
93:
89:
88:
85:
82:
80:
79:Constellation
77:
76:
73:
70:
66:
63:
57:
53:
52:
47:
40:
34:
19:
1806:WISE objects
1786:Brown dwarfs
1623:HD 196885 Ab
1586:
1462:
1369:
1366:
1337:ε (Aldulfin)
1312:α (Sualocin)
1196:
1190:
1150:
1146:
1136:
1093:
1089:
1079:
1036:
1032:
967:
961:
895:
889:
834:
828:
769:
717:
715:
695:
611:
595:
592:Space motion
552:
546:
535:
526:
511:
501:
497:
494:
459:
455:
454:
440:
377:
362:
357:
346:
337:
326:
317:
283:
267:
216:
49:
45:
1618:HD 195019 b
1425:18 (Musica)
1317:β (Rotanev)
844:1108.4677v1
739:(Y0 (pec?))
516:brown dwarf
509:Kirkpatrick
476:light-years
464:brown dwarf
379:Temperature
105:Declination
98:20 56 28.88
1780:Categories
1605:Exoplanets
1199:(2): 119.
977:2011.11616
898:(2): 156.
781:References
663:-free and
429:2056+1459
424:J2056+1459
419:J2056+1459
361:(log
206:Astrometry
1796:Delphinus
1654:Laevens 3
1382:Flamsteed
1206:1211.6977
1177:2515-5172
1153:(1): 13.
1128:0004-637X
1103:1212.1210
1046:1108.4678
1039:(1): 50.
1004:227126954
930:119279752
905:1205.2122
837:(2): 19.
661:phosphine
583:0.3
572:0.1
561:2.0
491:Discovery
472:Delphinus
189: (H
181:>17.1
170: (H
151: (J
143:>17.6
132: (J
84:Delphinus
1767:Category
1747:ZW II 96
1704:Galaxies
1690:NGC 6905
1664:NGC 7006
1659:NGC 6934
1435:Variable
1370:(Tso Ke)
1231:42923100
970:(1): 7.
869:16850733
692:See also
665:diabatic
655:and the
633:chloride
618:88
543:Distance
525:Cushing
285:Distance
269:Parallax
1682:Nebulae
1628:WASP-2b
1211:Bibcode
1155:Bibcode
1108:Bibcode
1096:: 130.
1051:Bibcode
982:Bibcode
910:Bibcode
849:Bibcode
696:Lists:
653:NIRSpec
645:methane
637:ammonia
629:sulfide
462:) is a
308:Details
69:Equinox
1577:WASP-2
1556:195019
1464:QV Sge
1368:ρ Aql
1229:
1175:
1126:
1071:286881
1069:
1002:
928:
867:
745:(Y0.5)
727:(T9.5)
625:Gemini
553:et al.
527:et al.
512:et al.
442:SIMBAD
417:WISEPC
412:WISEPC
391:
339:Radius
255:
247:
235:
227:
51:unWISE
46:Credit
1740:Other
1565:Other
1304:Bayer
1295:Stars
1227:S2CID
1201:arXiv
1098:arXiv
1067:S2CID
1041:arXiv
1000:S2CID
972:arXiv
926:S2CID
900:arXiv
865:S2CID
839:arXiv
762:Notes
757:(≥Y2)
598:980.6
577:, or
557:140.8
480:Earth
478:from
249:528.8
245:Dec.:
229:825.8
174:2MASS
136:2MASS
72:J2000
62:Epoch
1731:7028
1726:7025
1721:7003
1538:8044
1533:8010
1528:7975
1523:7907
1518:7899
1513:7839
1508:7824
1503:7816
1498:7793
1493:7778
1488:7774
1483:7771
1458:V339
1173:ISSN
1124:ISSN
751:(Y0)
733:(Y0)
631:and
579:23.2
500:and
448:data
427:WISE
422:WISE
319:Mass
1713:NGC
1219:doi
1197:762
1163:doi
1116:doi
1094:763
1059:doi
1037:743
990:doi
968:253
918:doi
896:753
857:doi
835:197
677:Myr
647:(CH
639:(NH
614:464
602:1.1
568:7.1
563:mas
466:of
385:464
371:cgs
350:Jup
330:Jup
277:mas
271:(π)
257:mas
253:0.8
237:mas
233:0.8
225:RA:
220:(μ)
193:MKO
155:MKO
124:Y0
65:MJD
1782::
1548:HD
1475:HR
1453:HU
1448:HR
1443:EU
1420:17
1415:16
1410:15
1405:14
1400:13
1395:10
1225:.
1217:.
1209:.
1195:.
1171:.
1161:.
1149:.
1145:.
1122:.
1114:.
1106:.
1092:.
1088:.
1065:.
1057:.
1049:.
1035:.
1012:^
998:.
988:.
980:.
966:.
960:.
938:^
924:.
916:.
908:.
894:.
877:^
863:.
855:.
847:.
833:.
788:^
720::
588:.
585:ly
574:pc
555::
482:.
389:88
297:pc
292:ly
261:yr
241:yr
197:)
178:)
159:)
140:)
48::
1390:1
1362:κ
1357:ι
1352:θ
1347:η
1342:ζ
1332:δ
1327:γ
1322:γ
1261:e
1254:t
1247:v
1233:.
1221::
1213::
1203::
1179:.
1165::
1157::
1151:8
1130:.
1118::
1110::
1100::
1073:.
1061::
1053::
1043::
1006:.
992::
984::
974::
932:.
920::
912::
902::
871:.
859::
851::
841::
685:J
682:M
649:4
641:3
620:K
616:±
600:±
581:±
570:±
559:±
538:.
393:K
387:±
365:)
363:g
347:R
327:M
299:)
259:/
251:±
239:/
231:±
191:(
172:(
153:(
134:(
20:)
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