28:
672:
2350:
564:). The follow-up study found that a single disk had a poor match with the 22 μm data. The researchers found a better match with a "warm" outer disk with a temperature of about 240 K (-33 °C or -28 °F) and a "hot" inner disk with a temperature of about 1100 K (827 °C or 1520 °F). The warm outer disk is located around 0.115
1144:
Silverberg, Steven M.; Wisniewski, John P.; Kuchner, Marc J.; Lawson, Kellen D.; Bans, Alissa S.; Debes, John H.; Biggs, Joseph R.; Bosch, Milton K. D.; Doll, Katharina; Luca, Hugo A. Durantini; Enachioaie, Alexandru; Hamilton, Joshua; Holden, Jonathan; Hyogo, Michiharu; the Disk
Detective
636:. The missing CO detection is explained with two possible scenarios: Either dust grains are released in a collisional cascade induced by the collisions of km-sized planetesimals or a recent collision of planetary bodies generated a large amount of small dust grains.
484:. Since most M-dwarf debris disks fade in less than 30 million years, this would be the oldest M dwarf debris disk detected in a moving group, implying a change in understanding of constraint in M-dwarf debris disk evolution.
655:
Other stars and brown dwarfs were discovered to be similar to J0808, with signs of youth while being in an older moving group. Together with J0808, these older low-mass accretors in nearby moving groups are being called
842:
Silverberg, Steven M.; Kuchner, Marc J.; Wisniewski, John P.; Gagné, Jonathan; Bans, Alissa S.; Bhattacharjee, Shambo; Currie, Thayne R.; Debes, John R.; Biggs, Joseph R. (14 October 2016).
568:
and the hot inner disk is located around 0.0056 au. The hot inner disk is likely the source of accreted material. The temperature of the inner disk is comparable to temperatures where
607:
detected a third component with a temperature of 20 K (-253 °C or -424 °F). Using this temperature the researchers were able to estimate the dust mass to 0.057±0.006
590:. The warm outer disk could be similar to dust belts seen around B- to K-type stars, which have temperatures around 190 K and which likely represent small dust grains of
671:
2392:
1259:
640:
525:
1041:
644:
1252:
2372:
2382:
2353:
1245:
55:
2276:
604:
591:
517:
492:
2377:
2320:
549:
1284:
725:
426:
1821:
1361:
504:
27:
361:
1279:
1747:
1268:
404:
116:
2387:
2196:
2012:
1584:
909:
Gaia
Collaboration (2018-08-01). "Gaia Data Release 2 - Summary of the contents and survey properties".
293:
1168:
1093:
996:
975:"A self-consistent, absolute isochronal age scale for young moving groups in the solar neighbourhood"
928:
865:
793:
478:
393:
229:
68:
2226:
710:
1816:
437:, discovered a debris disk around J0808, using the WISE telescope, a M5.5V dwarf with significant
1186:
1158:
1119:
1083:
1022:
986:
952:
918:
891:
855:
819:
783:
397:
2211:
1303:
1111:
1014:
944:
883:
811:
633:
575:
565:
458:
308:
104:
51:
1176:
1101:
1004:
936:
932:
873:
844:"A New M Dwarf Debris Disk Candidate in a Young Moving Group Discovered with Disk Detective"
801:
206:
974:
629:
1341:
1321:
730:
569:
521:
462:
430:
138:
76:
1172:
1097:
1000:
869:
797:
2302:
2294:
1831:
1826:
1231:
770:
Flaherty, Kevin; Hughes, A. Meredith; Mamajek, Eric E.; Murphy, Simon J. (2019-02-13).
715:
694:
689:
657:
621:
446:
434:
335:
221:
194:
174:
1204:
878:
843:
2366:
2191:
2076:
1351:
1331:
1190:
1123:
1072:"WISE J080822.18−644357.3 – a 45 Myr-old accreting M dwarf hosting a primordial disc"
895:
823:
537:
533:
481:
155:
63:
1026:
956:
2111:
2001:
1962:
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1952:
1947:
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1937:
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1539:
1529:
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1469:
1464:
1459:
1449:
1336:
1316:
720:
598:
587:
488:
263:
940:
643:
shows variations, which could be disk material blocking light from the star. The
2333:
2106:
2101:
2096:
1982:
1866:
1861:
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1841:
1569:
1564:
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1549:
1346:
1326:
705:
583:
400:
389:
89:
1181:
1146:
806:
771:
586:
of the red dwarf and therefore the inner disk could be the result of disrupted
2328:
2201:
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1987:
1977:
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407:
109:
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1071:
677:
Spectral Energy
Distribution (SED) of J0808 (from Disk Detective talk page)
524:, but unresolved 1.3 mm dust emission was detected. Observations with
1237:
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2206:
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699:
572:
474:
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324:
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1836:
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1687:
1637:
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1504:
1311:
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557:
500:
496:
1070:
Murphy, Simon J.; Mamajek, Eric E.; Bell, Cameron P. M. (2018-05-21).
772:"The Planet Formation Potential around a 45 Myr Old Accreting M Dwarf"
2245:
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2125:
1911:
1906:
1901:
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553:
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355:
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241:
1042:"Citizen Scientists Discover Potential New Exoplanet Hunting Ground"
1163:
1088:
991:
923:
860:
788:
1896:
1891:
1886:
1147:"Peter Pan Disks: Long-lived Accretion Disks Around Young M Stars"
415:
973:
Bell, Cameron P. M.; Mamajek, Eric E.; Naylor, Tim (2015-11-21).
647:
light curve shows aperiodic dipping on timescales of 0.5–2 days.
1294:
422:
386:
198:
178:
39:
1241:
617:
594:
702:
another system discovered by Disk
Detective volunteers
2319:
2293:
2269:
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2184:
2133:
2124:
2059:
2011:
2000:
1928:
1804:
1746:
1583:
1360:
1302:
1293:
552:of J0808 indicates a disk temperature of about 263
1076:Monthly Notices of the Royal Astronomical Society
979:Monthly Notices of the Royal Astronomical Society
616:. This is higher than the disk mass around ~20
1253:
461:revealed (with 93.9% probability) the star's
8:
837:
835:
833:
503:emission. The data is consistent with a low
540:lines, which is a clear sign of accretion.
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2130:
2008:
1925:
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747:
94:−64° 43′ 57.3″
16:Red dwarf star in the constellation Carina
1180:
1162:
1105:
1087:
1008:
990:
922:
877:
859:
805:
787:
54:J2000
32:Artist's depiction of J080822.18-644357.3
632:. The disk has a radius smaller than 16
582:form. The inner disk also lies near the
2393:Astronomical objects discovered in 2016
1205:"Low-mass Stars | Steven M. Silverberg"
743:
667:
548:The fitting of a modeled disk with the
162:
18:
493:ANU Siding Spring 2.3 meter telescope
7:
1139:
1137:
1135:
1133:
1065:
1063:
1061:
628:, but smaller than the ~10 Myr old
473:, associating it with Carina's ~45
182:
14:
453:in the project database—or
2349:
2348:
670:
520:observations did not detect any
26:
2277:Carina Dwarf Spheroidal Galaxy
1:
1145:Collaboration (2020-01-14).
1040:Ramsey, Sarah (2016-10-21).
911:Astronomy & Astrophysics
550:Spectral Energy Distribution
457:for short—a BANYAN II
1285:Carina in Chinese astronomy
941:10.1051/0004-6361/201833051
879:10.3847/2041-8205/830/2/L28
726:Goddard Space Flight Center
427:Goddard Space Flight Center
2409:
2373:M-type main-sequence stars
499:-rich M5-star with strong
487:A follow-up study with an
2346:
2315:
2289:
1924:
1275:
1151:The Astrophysical Journal
848:The Astrophysical Journal
776:The Astrophysical Journal
441:excess at both 12 and 22
348:
343:WISE J080822.18-644357.3
341:
334:
330:
257:
252:
248:
132:
125:
98:
48:
24:
1182:10.3847/1538-4357/ab68e6
807:10.3847/1538-4357/aaf794
370:WISE J080822.18-644357.3
1280:List of stars in Carina
1269:Constellation of Carina
933:2018A&A...616A...1G
105:Evolutionary stage
2383:Carina (constellation)
532:and variations in the
2197:Finger of God Globule
1988:HD 95086 b (Levantes)
1010:10.1093/mnras/stv1981
421:On October 21, 2016,
1234:at diskdetective.org
1232:AWI0005x3s talk page
1107:10.1093/mnras/sty471
624:and the ~50 Myr old
394:Carina constellation
149:22.7 ± 0.5 km/s
20:J080822.18-644357.3
2378:Circumstellar disks
2321:Astronomical events
1173:2020ApJ...890..106S
1098:2018MNRAS.476.3290M
1001:2015MNRAS.454..593B
870:2016ApJ...830L..28S
798:2019ApJ...872...92F
711:Protoplanetary disk
639:A light curve from
429:announced that its
349:Database references
21:
1968:HD 63765 b (Yvaga)
491:obtained with the
336:Other designations
240:(101.4 ± 0.6
117:Spectral type
19:
2360:
2359:
2342:
2341:
2311:
2310:
2285:
2284:
2240:
2239:
2212:Homunculus Nebula
2120:
2119:
1996:
1995:
1920:
1919:
459:Bayesian analysis
367:
366:
2400:
2352:
2351:
2317:
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2131:
2009:
1926:
1380:T (not variable)
1300:
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1215:
1201:
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1194:
1184:
1166:
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1128:
1127:
1109:
1091:
1082:(3): 3290–3302.
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809:
791:
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528:showed a strong
489:optical spectrum
445:. Classified as
384:
383:
322:
321:
299:3050 ± 100
278:
277:
276:
219:
217:
192:
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172:
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99:Characteristics
84:
79:
49:Observation data
42:/Jonathan Holden
30:
22:
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2295:Galaxy clusters
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2265:
2236:
2227:IGR J11014−6103
2180:
2116:
2055:
2003:
1992:
1916:
1800:
1761:63765 (Tapecue)
1742:
1579:
1356:
1317:β (Miaplacidus)
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731:Citizen science
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658:Peter Pan disks
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651:Peter Pan disks
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522:carbon monoxide
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463:radial velocity
431:citizen science
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77:Right ascension
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2303:Bullet Cluster
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1226:External links
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1220:
1209:www.nhn.ou.edu
1196:
1129:
1057:
1032:
985:(1): 593–614.
962:
901:
829:
742:
741:
739:
736:
734:
733:
728:
723:
718:
716:Accretion disk
713:
708:
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697:
695:Disk Detective
692:
690:Peter Pan Disk
686:
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669:
665:
662:
652:
649:
622:AU Microscopii
612:
609:
545:
542:
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465:as 20.6 ± 1.4
447:Peter Pan disk
435:Disk Detective
380:
372:, also called
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2200:
2198:
2195:
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2192:Carina Nebula
2190:
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2177:
2174:
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2077:Collinder 228
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1823:
1822:DEN 0817−6155
1820:
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599:planetesimals
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398:circumstellar
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156:Proper motion
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67:
65:
64:Constellation
62:
61:
57:
53:
47:
43:
41:
36:
29:
23:
2388:WISE objects
2112:Westerlund 2
1963:OGLE2-TR-L9b
1958:OGLE-TR-211b
1953:OGLE-TR-182b
1948:OGLE-TR-113b
1943:OGLE-TR-132b
1938:OGLE-TR-111b
1811:
1212:. Retrieved
1208:
1199:
1154:
1150:
1079:
1075:
1049:. Retrieved
1045:
1035:
982:
978:
914:
910:
904:
851:
847:
779:
775:
721:T Tauri star
654:
638:
603:
547:
486:
482:moving group
454:
450:
420:
403:orbiting an
373:
369:
368:
354:
307:
292:
262:
228:
205:
154:
137:
38:
34:
2334:GRB 080916C
2107:Trumpler 16
2102:Trumpler 15
2097:Trumpler 14
1983:HD 85628 Ab
1867:OGLE2-TR-L9
1862:OGLE-TR-211
1857:OGLE-TR-182
1842:NGC 3603-A1
1832:Innes' star
1817:CPD−57°2874
1312:α (Canopus)
706:Debris disk
592:sublimating
584:Roche limit
580:crystalline
544:Debris disk
401:debris disk
294:Temperature
90:Declination
83:08 08 22.18
2367:Categories
2329:GRB 000131
2202:G290.1-0.8
2072:Carina OB2
2067:Carina OB1
1978:HD 65216 c
1973:HD 65216 b
1930:Exoplanets
1852:NGC 3603-C
1847:NGC 3603-B
1827:1E 1048-59
1812:AWI0005x3s
1214:2019-07-25
1164:2001.05030
1157:(2): 106.
1089:1703.04544
1051:2020-01-08
992:1508.05955
924:1804.09365
861:1610.05293
854:(2): L28.
789:1812.04124
738:References
538:Brackett-γ
451:AWI0005x3s
412:lightyears
410:about 331
127:Astrometry
2092:Platais 8
1322:ε (Avior)
1191:210718358
1124:119341475
1116:0035-8711
1019:0035-8711
949:0004-6361
896:119183849
888:2041-8205
824:119251811
816:1538-4357
782:(1): 92.
597:from icy
573:silicates
570:amorphous
534:Paschen-β
505:accretion
495:showed a
433:project,
408:red dwarf
376:, is a 45
235:331
110:red dwarf
2354:Category
2246:Galaxies
2207:Hen 2-47
2004:clusters
1738:4325 (z)
1733:4257 (u)
1718:4177 (t)
1713:4164 (t)
1708:4159 (r)
1698:4138 (K)
1693:4114 (s)
1688:4102 (I)
1683:4089 (L)
1678:4025 (M)
1673:3884 (l)
1668:3856 (m)
1663:3825 (h)
1658:3821 (H)
1653:3728 (k)
1648:3696 (g)
1643:3663 (i)
1638:3643 (G)
1633:3598 (b)
1628:3571 (c)
1623:3415 (e)
1618:3414 (e)
1613:3260 (C)
1608:3220 (B)
1603:3159 (D)
1598:2934 (Q)
1593:2435 (N)
1530:V533 (y)
1520:V520 (w)
1510:V448 (O)
1505:V415 (A)
1500:V399 (P)
1495:V382 (x)
1490:V376 (b)
1480:V371 (z)
1475:V357 (a)
1470:V345 (E)
1465:V344 (f)
1460:V343 (d)
1450:V337 (q)
1362:Variable
1027:55297862
957:49211658
700:HD 74389
683:See also
613:☉
513:☉
439:infrared
385:Myr old
285:☉
230:Distance
207:Parallax
2222:IC 2448
2217:IC 2220
2126:Nebulae
2087:IC 2714
2082:IC 2602
1872:Sher 25
1837:LHS 288
1169:Bibcode
1094:Bibcode
997:Bibcode
929:Bibcode
866:Bibcode
794:Bibcode
664:Gallery
449:number
396:with a
392:in the
253:Details
56:Equinox
2232:RCW 49
1912:WR 42e
1907:WR 31a
1902:WR 30a
1882:WR 21a
1877:WR 20a
1440:PP (p)
1189:
1122:
1114:
1025:
1017:
955:
947:
917:: A1.
894:
886:
822:
814:
626:GJ 182
576:anneal
560:or 14
507:of 10
405:M-type
390:system
356:SIMBAD
323:
279:
220:
218:0.0551
214:9.8599
193:
185:
173:
167:−11.54
165:
121:M5.5V
69:Carina
58:J2000
35:Credit
2270:Other
2185:Other
2060:Other
1897:WR 25
1892:WR 24
1887:WR 22
1805:Other
1796:97950
1791:95086
1786:93403
1781:93250
1776:93129
1771:85628
1766:65216
1756:53143
1304:Bayer
1295:Stars
1187:S2CID
1159:arXiv
1120:S2CID
1084:arXiv
1023:S2CID
987:arXiv
953:S2CID
919:arXiv
892:S2CID
856:arXiv
820:S2CID
784:arXiv
630:TWA 7
578:into
556:(-10
530:flare
516:yr .
479:young
416:Earth
414:from
374:J0808
275:−0.04
273:+0.03
187:25.61
183:Dec.:
52:Epoch
2261:3059
2176:3586
2171:3584
2166:3582
2161:3581
2156:3579
2151:3576
2146:3199
2141:2867
2051:3603
2046:3532
2041:3324
2036:3293
2031:3114
2026:2808
2021:2516
2002:Star
1728:4222
1723:4205
1703:4142
1575:V906
1570:V817
1565:V816
1560:V759
1555:V752
1550:V742
1545:V640
1540:V602
1535:V560
1525:V528
1515:V518
1485:V372
1455:V341
1112:ISSN
1046:NASA
1015:ISSN
945:ISSN
884:ISSN
812:ISSN
645:TESS
641:CTIO
620:old
605:ALMA
536:and
526:CTIO
518:ALMA
477:old
455:5x3s
423:NASA
387:star
362:data
270:0.16
264:Mass
191:0.10
171:0.12
40:NASA
2254:NGC
2134:NGC
2013:NGC
1177:doi
1155:890
1102:doi
1080:476
1005:doi
983:454
937:doi
915:616
874:doi
852:830
802:doi
780:872
618:Myr
595:ice
475:Myr
425:'s
325:Myr
309:Age
222:mas
209:(π)
195:mas
175:mas
163:RA:
158:(μ)
2369::
1748:HD
1585:HR
1445:QZ
1435:OY
1430:IX
1425:HR
1420:GG
1415:EV
1410:CK
1405:BO
1400:AG
1395:RT
1207:.
1185:.
1175:.
1167:.
1153:.
1149:.
1132:^
1118:.
1110:.
1100:.
1092:.
1078:.
1074:.
1060:^
1044:.
1021:.
1013:.
1003:.
995:.
981:.
977:.
965:^
951:.
943:.
935:.
927:.
913:.
890:.
882:.
872:.
864:.
850:.
846:.
832:^
818:.
810:.
800:.
792:.
778:.
774:.
746:^
660:.
634:au
601:.
566:au
562:°F
558:°C
501:Hα
497:Li
467:km
443:μm
418:.
381:−7
319:−7
314:45
242:pc
237:ly
199:yr
179:yr
141:(R
37::
1390:Y
1385:U
1375:S
1370:R
1352:ω
1347:χ
1342:υ
1332:θ
1327:η
1261:e
1254:t
1247:v
1217:.
1193:.
1179::
1171::
1161::
1126:.
1104::
1096::
1086::
1054:.
1029:.
1007::
999::
989::
959:.
939::
931::
921::
898:.
876::
868::
858::
826:.
804::
796::
786::
610:M
554:K
510:M
471:s
469:/
301:K
282:M
244:)
216:±
197:/
189:±
177:/
169:±
145:)
143:v
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