113:
2623:
520:
Schneider, Donald P.; Fan, Xiaohui; Hall, Patrick B.; Jester, Sebastian; Richards, Gordon T.; Stoughton, Chris; Strauss, Michael A.; SubbaRao, Mark; Vanden Berk, Daniel E.; Anderson, Scott F.; Brandt, W. N.; Gunn, James E.; Gray, Jim; Trump, Jonathan R.; Voges, Wolfgang (2003-12-01).
578:
Morabito, L. K.; Matthews, J. H.; Best, P. N.; Gürkan, G.; Jarvis, M. J.; Prandoni, I.; Duncan, K. J.; Hardcastle, M. J.; Kunert-Bajraszewska, M.; Mechev, A. P.; Mooney, S.; Sabater, J.; Röttgering, H. J. A.; Shimwell, T. W.; Smith, D. J. B. (2019-02-01).
636:
Trump, Jonathan R.; Hall, Patrick B.; Reichard, Timothy A.; Richards, Gordon T.; Schneider, Donald P.; Vanden Berk, Daniel E.; Knapp, Gillian R.; Anderson, Scott F.; Fan, Xiaohui; Brinkman, J.; Kleinman, S. J.; Nitta, Atsuko (2006-07-01).
694:
Hall, P. B.; Brandt, W. N.; Petitjean, P.; Pâris, I.; Filiz Ak, N.; Shen, Yue; Gibson, R. R.; Aubourg, É.; Anderson, S. F.; Schneider, D. P.; Bizyaev, D.; Brinkmann, J.; Malanushenko, E.; Malanushenko, V.; Myers, A. D. (2013-09-01).
496:
31:
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754:
Filbert, S.; Martini, P.; Seebaluck, K.; Ennesser, L.; Alexander, D. M.; Bault, A.; Brodzeller, A.; Herrera-Alcantar, H. K.; Montero-Camacho, P. (2023-09-06).
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Feel free to improve the article, but do not remove this notice before the discussion is closed. For more information, see the
391:, but also compromise cosmological studies, which the quasars are studied for their impact on accurate redshifts as well as
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Bower, R. G.; Benson, A. J.; Malbon, R.; Helly, J. C.; Frenk, C. S.; Baugh, C. M.; Cole, S.; Lacey, C. G. (2006-08-01).
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Such of these broad absorption line quasars like SDSS J082535.19+512706.3 have a unique morphology, which they contain
53:
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1037:
697:"Broad absorption line quasars with redshifted troughs: high-velocity infall or rotationally dominated outflows?"
36:
326:
277:
118:
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have higher velocities more than 0.1c. These makes them interesting as they provide signatures of significant
581:"The origin of radio emission in broad absorption line quasars: Results from the LOFAR Two-metre Sky Survey"
439:
411:
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that leads to large amounts of outflows pouring out from the quasar's center. This potentially affects the
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639:"A Catalog of Broad Absorption Line Quasars from the Sloan Digital Sky Survey Third Data Release"
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Zuo, Wenwen; Wu, Xue-Bing; Fan, Xiaohui; Green, Richard; Wang, Ran; Bian, Fuyan (2015-01-28).
905:
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756:"Broad Absorption Line Quasars in the Dark Energy Spectroscopic Instrument Early Data Release"
736:
676:
618:
560:
450:. These signs indicates that SDSS J082535.19+512706.3 is in the process of rapid enlargement.
341:
with FWHM larger than 1000 km s-1, with high redshifts ranging from 0.08 to 5.41, with a
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with H0=70 km s-1 Mpc-1, ΩM=0.3, and ΩΛ=0.7). These quasars also contain at least one
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According to researchers, it has been proposed SDSS J082535.19+512706.3 might have gone a
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928:"BLACK HOLE MASS ESTIMATES AND RAPID GROWTH OF SUPERMASSIVE BLACK HOLES IN LUMINOUS
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of v ≃ 12 000 km s, with its widths exceeding at least 3000 km s.
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trough, including an absorption redshift that is relative to the quasar's
91:%5B%5BWikipedia%3AArticles+for+deletion%2FSDSS+J082535.19%2B512706.3%5D%5D
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in the center of SDSS J082535.19+512706.3 is surrounded by a luminous
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523:"The Sloan Digital Sky Survey Quasar Catalog. II. First Data Release"
469:
ratio, the black hole in SDSS J082535.19+512706.3 is found to have a
342:
305:
is 3.495596, which corresponds the object to be located 11.5 billion
294:
772:
672:
597:
556:
473:
of (1.12 + 0.20) x 10. This makes the quasar to contain one of the
321:
SDSS J082535.19+512706.3 was first discovered in 2003 by a team of
1900:
1895:
948:
713:
310:
269:
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J082535.19+5127062, WISEA J082535.19+512706.3, LQAC 126+051 006,
1854:
1849:
1047:
372:
994:
866:"The hierarchical formation of the brightest cluster galaxies"
438:
From the study conducted by researchers, it is found that the
18:
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1979:
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864:De Lucia, Gabriella; Blaizot, Jérémy (2007-02-01).
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348:SDSS J082535.19+512706.3 is classified as a broad
26:An editor has nominated this article for deletion.
870:Monthly Notices of the Royal Astronomical Society
811:Monthly Notices of the Royal Astronomical Society
760:Monthly Notices of the Royal Astronomical Society
701:Monthly Notices of the Royal Astronomical Society
446:, in which the quasar radiates hot amounts of
325:, whom they presented 16,713 objects from the
1006:
461:emissions, which the said lines were used by
8:
807:"Breaking the hierarchy of galaxy formation"
643:The Astrophysical Journal Supplement Series
360:. Its redshifted trough extends upwards to
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1976:
1940:
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280:J082535.18+512706.3, KODIAQ J082535+512706
111:
947:
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881:
840:
822:
789:
771:
730:
712:
654:
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453:Moreover, SDSS J082535.19+512706.3 is a
215:
117:The quasar SDSS J082535.19+512706.3 via
485:
352:quasar, specifically containing a high
329:First Data Release which contain high
102:
465:to study its black hole. Through the
7:
2666:Principal Galaxies Catalogue objects
921:
919:
491:
489:
229:
29:You are welcome to participate in
14:
2622:
2621:
901:10.1111/j.1365-2966.2006.11287.x
842:10.1111/j.1365-2966.2006.10519.x
399:distribution traceable by their
16:Quasar in the constellation Lynx
1:
297:located in the constellation
585:Astronomy & Astrophysics
457:quasar containing Mg II and
181:Heliocentric radial velocity
966:10.1088/0004-637x/799/2/189
615:10.1051/0004-6361/201833821
37:whether or not to retain it
2687:
54:"SDSS J082535.19+512706.3"
2619:
2588:
2542:
1939:
1913:
1867:
1038:Lynx in Chinese astronomy
1028:
936:The Astrophysical Journal
497:"Your NED Search Results"
268:
110:
2671:Supermassive black holes
2505:SDSS J082535.19+512706.3
527:The Astronomical Journal
475:most massive black holes
383:features although their
287:SDSS J082535.19+512706.3
119:Sloan Digital Sky Survey
106:SDSS J082535.19+512706.3
607:2019A&A...622A..15M
440:supermassive black hole
412:active galactic nucleus
32:the deletion discussion
791:10.1093/mnras/stae1610
1033:List of stars in Lynx
1022:Constellation of Lynx
732:10.1093/mnras/stt1012
2651:Lynx (constellation)
1886:WASP-13b (Cruinlagh)
501:ned.ipac.caltech.edu
35:, which will decide
2594:Astronomical events
2556:2XMM J083026+524133
958:2015ApJ...799..189Z
892:2007MNRAS.375....2D
833:2006MNRAS.370..645B
782:2024MNRAS.532.3669F
723:2013MNRAS.434..222H
665:2006ApJS..165....1T
549:2003AJ....126.2579S
420:interstellar medium
1901:XO-5b (Makropulos)
401:Lyman-alpha forest
333:than Mi=-22 (in a
264:Other designations
240:Surface brightness
226:Apparent magnitude
212:Apparent magnitude
126:Observation data (
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2571:Lynx Supercluster
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410:, triggering its
379:of common quasar
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43:guide to deletion
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1953:Jones-Emberson 1
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883:astro-ph/0606519
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533:(6): 2579–2593.
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1840:WASP-13 (Gloas)
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350:absorption line
345:value of 1.43.
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317:Characteristics
249:Characteristics
165:+51d 27m 06.40s
151:Right ascension
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932:∼ 3.5 QUASARS"
915:
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817:(2): 645–655.
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707:(1): 222–256.
686:
673:10.1086/503834
628:
570:
557:10.1086/379174
512:
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444:accretion disk
435:
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424:star formation
422:thus reducing
395:of the matter
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291:QSO J0825+5127
289:also known as
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155:08h 25m 35.19s
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1959:
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1919:Star clusters
1916:
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1016:
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983:
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945:
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933:
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867:
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848:
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648:
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632:
629:
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608:
604:
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582:
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571:
566:
562:
558:
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541:
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532:
528:
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516:
513:
502:
498:
492:
490:
486:
480:
478:
476:
472:
468:
464:
460:
456:
455:hyperluminous
451:
449:
445:
441:
433:
431:
429:
425:
421:
417:
413:
409:
408:galaxy merger
404:
402:
398:
394:
390:
386:
382:
378:
374:
370:
365:
363:
359:
355:
351:
346:
344:
340:
339:emission line
336:
332:
328:
324:
316:
314:
312:
308:
304:
300:
296:
292:
288:
279:
275:
271:
267:
262:
258:
256:
252:
247:
243:
241:
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233:
227:
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219:
213:
209:
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201:
197:
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188:
184:
182:
178:
174:
172:
168:
164:
162:
158:
154:
152:
148:
145:
142:
140:
139:Constellation
136:
132:
129:
124:
120:
114:
109:
104:
87:
84:
80:
77:
73:
70:
66:
63:
59:
56: –
55:
51:
50:Find sources:
44:
38:
34:
33:
27:
23:
21:
20:
2661:SDSS objects
2504:
1820:HS 0702+6043
1342:
1335:
1328:
1321:
1314:
1307:
1300:
1293:
1286:
1279:
1069:
939:
935:
929:
873:
869:
859:
814:
810:
800:
763:
759:
749:
704:
700:
689:
646:
642:
631:
588:
584:
573:
530:
526:
515:
504:. Retrieved
500:
452:
437:
405:
393:measurements
366:
347:
331:luminosities
320:
290:
286:
285:
82:
75:
68:
61:
49:
30:
25:
1850:XO-4 (Koit)
1835:PG 0859+415
876:(1): 2–14.
766:(4): 3669.
649:(1): 1–18.
428:host galaxy
418:make-up of
377:wavelengths
323:astronomers
307:light-years
161:Declination
2640:Categories
1881:6 Lyncis b
1873:Exoplanets
1830:J0815+4729
1825:IRC +60169
1805:Gliese 277
1071:ψ Aur (16)
974:1885/64781
942:(2): 189.
773:2309.03434
598:1811.07931
506:2024-05-27
481:References
471:solar mass
463:scientists
434:Black hole
385:blueshifts
371:absorbing
369:gas clouds
362:velocities
358:rest frame
354:ionization
185:1,047,953
65:newspapers
2602:SN 2007uy
2566:Abell 576
2561:Abell 569
1082:Flamsteed
982:1538-4357
949:1412.2438
910:0035-8711
851:0035-8711
741:0035-8711
714:1306.2680
681:0067-0049
623:0004-6361
565:0004-6256
467:Eddington
335:cosmology
276:4042723,
206:distance)
2627:Category
2607:SN 2008D
2530:UGC 4904
2525:UGC 4881
2520:UGC 4653
1972:Galaxies
1958:Lynx Arc
1927:NGC 2666
1355:Variable
416:chemical
389:feedback
381:spectral
303:redshift
194:Distance
175:3.495596
171:Redshift
2646:Quasars
2510:IC 2233
1945:Nebulae
1815:GJ 3421
1810:GJ 1105
954:Bibcode
888:Bibcode
829:Bibcode
778:Bibcode
719:Bibcode
661:Bibcode
603:Bibcode
591:: A15.
545:Bibcode
426:in its
397:density
293:, is a
198:11.503
128:J2000.0
79:scholar
2495:3C 171
1891:XO-2Nb
1344:19 UMa
1337:10 UMa
1323:54 Cam
1316:52 Cam
1309:50 Cam
1302:48 Cam
1295:46 Cam
1288:45 Cam
1281:44 Cam
980:
908:
849:
739:
679:
621:
563:
343:median
301:. Its
295:quasar
228:
214:
81:
74:
67:
60:
52:
2488:Other
2319:2719A
2254:2537A
2089:2429B
2084:2429A
2029:2326A
1994:2273B
1800:GD 98
1793:Other
1779:67539
1774:65392
1769:63630
1764:63588
1759:59826
1754:59721
1749:58681
1744:52859
1739:48948
1734:44061
1330:5 LMi
1057:Bayer
1048:Stars
944:arXiv
878:arXiv
819:arXiv
768:arXiv
709:arXiv
651:arXiv
593:arXiv
535:arXiv
311:Earth
309:from
270:2MASS
259:HiBAL
131:epoch
86:JSTOR
72:books
2479:2860
2474:2853
2469:2852
2464:2844
2459:2840
2454:2839
2449:2838
2444:2834
2439:2833
2434:2832
2429:2831
2424:2830
2419:2829
2414:2828
2409:2827
2404:2826
2399:2825
2394:2823
2389:2799
2384:2798
2379:2793
2374:2785
2369:2782
2364:2780
2359:2779
2354:2778
2349:2776
2344:2770
2339:2759
2334:2755
2329:2746
2324:2724
2314:2719
2309:2712
2304:2704
2299:2691
2294:2683
2289:2668
2284:2649
2279:2638
2274:2552
2269:2549
2264:2543
2259:2541
2249:2537
2244:2534
2239:2532
2234:2528
2229:2524
2224:2521
2219:2519
2214:2518
2209:2505
2204:2500
2199:2497
2194:2495
2189:2493
2184:2488
2179:2484
2174:2476
2169:2475
2164:2474
2159:2473
2154:2472
2149:2469
2144:2468
2139:2463
2134:2462
2129:2461
2124:2458
2119:2457
2114:2456
2109:2446
2104:2445
2099:2444
2094:2431
2079:2429
2074:2426
2069:2424
2064:2415
2059:2344
2054:2340
2049:2337
2044:2332
2039:2330
2034:2329
2024:2326
2019:2322
2014:2321
2009:2320
2004:2315
1999:2308
1989:2273
1845:XO-2
1716:3809
1711:3701
1706:3686
1701:3625
1696:3612
1691:3586
1686:3580
1681:3546
1676:3545
1671:3511
1666:3509
1661:3360
1656:3351
1651:3348
1646:3309
1641:3292
1636:3287
1631:3277
1626:3258
1621:3246
1616:3200
1611:3181
1606:3175
1601:3130
1596:3106
1591:3094
1586:3039
1581:3028
1576:2939
1571:2935
1566:2915
1561:2914
1556:2903
1551:2894
1546:2844
1541:2804
1536:2776
1531:2751
1526:2737
1521:2721
1516:2645
1511:2642
1506:2561
1501:2486
1496:2463
978:ISSN
906:ISSN
847:ISSN
737:ISSN
677:ISSN
619:ISSN
561:ISSN
373:flux
327:SDSS
299:Lynx
278:SDSS
255:Type
244:19.3
234:0.18
220:0.13
187:km/s
144:Lynx
58:news
1981:NGC
970:hdl
962:doi
940:799
896:doi
874:375
837:doi
815:370
786:doi
764:532
727:doi
705:434
669:doi
647:165
611:doi
589:622
553:doi
531:126
375:at
274:PGC
230:(B)
216:(V)
200:Gly
94:AFD
2642::
1726:HD
1488:HR
1478:DU
1473:DI
1468:DD
1463:CY
1458:CC
1453:BK
1448:BH
1443:BF
1438:BE
1433:AN
1428:UY
1423:UX
1418:UV
1413:UU
1408:TZ
1403:TV
1398:TT
1393:SZ
1388:SW
1383:RR
1275:43
1270:42
1265:38
1260:36
1255:35
1250:34
1245:33
1240:32
1230:30
1225:29
1220:28
1215:27
1210:26
1205:25
1200:24
1195:23
1190:22
1185:21
1180:20
1175:19
1170:18
1165:17
1160:15
1155:14
1150:13
1145:12
1140:11
1135:10
976:.
968:.
960:.
952:.
938:.
934:.
918:^
904:.
894:.
886:.
872:.
868:.
845:.
835:.
827:.
813:.
809:.
784:.
776:.
762:.
758:.
735:.
725:.
717:.
703:.
699:.
675:.
667:.
659:.
645:.
641:.
617:.
609:.
601:.
587:.
583:.
559:.
551:.
543:.
529:.
525:.
499:.
488:^
477:.
459:Hβ
430:.
403:.
313:.
1378:Y
1373:U
1368:T
1363:R
1130:9
1125:8
1120:7
1115:6
1110:5
1105:4
1100:3
1095:2
1090:1
1065:α
1014:e
1007:t
1000:v
984:.
972::
964::
956::
946::
930:z
912:.
898::
890::
880::
853:.
839::
831::
821::
794:.
788::
780::
770::
743:.
729::
721::
711::
683:.
671::
663::
653::
625:.
613::
605::
595::
567:.
555::
547::
537::
509:.
202:(
133:)
83:·
76:·
69:·
62:·
45:.
39:.
Text is available under the Creative Commons Attribution-ShareAlike License. Additional terms may apply.
