32:
2232:
39:
1280:
1138:
1275:{\displaystyle {\begin{aligned}2\cdot R_{*}&={\frac {(10^{-3}\cdot 49.2\cdot 3.003)\ {\text{AU}}}{0.0046491\ {\text{AU}}/R_{\bigodot }}}\\&\approx 31.78\cdot R_{\bigodot }\end{aligned}}}
1143:
649:(WGSN) to catalog and standardize proper names for stars. The WGSN's first bulletin of July 2016 included a table of the first two batches of names approved by the WGSN; which included
1298:
da Silva, Ronaldo; Milone, André de C.; Rocha-Pinto, Helio J. (2015-08-01). "Homogeneous abundance analysis of FGK dwarf, subgiant, and giant stars with and without giant planets".
526:
1551:
1699:
792:
952:
930:
394:
1794:
742:
and it is about 240 million years old, which is the sufficient time for a star this massive to consume the hydrogen at its core and evolve away from the
70:
1051:
Lyubimkov, Leonid S.; et al. (February 2010), "Accurate fundamental parameters for A-, F- and G-type
Supergiants in the solar neighbourhood",
971:
Determination of Radial
Velocities and their Applications, Proceedings from IAU Symposium no. 30 held at the University of Toronto 20-24 June, 1966
2284:
2299:
1599:
1533:
1395:
1697:
Roberts, Lewis C. Jr. (May 2011), "Astrometric and photometric measurements of binary stars with adaptive optics: observations from 2002",
1787:
969:
Evans, D. S. (1967), "The
Revision of the General Catalogue of Radial Velocities", in Batten, Alan Henry; Heard, John Frederick (eds.),
674:
1123:
2254:
948:
642:
1616:"A list of bright interferometric calibrators measured at the European Southern Observatory Very Large Telescope Interferometer"
2294:
1548:
646:
63:
2259:
2235:
1780:
1433:
530:
2264:
446:
807:
of 1.4°. Component B has been observed to fluctuate in brightness and is catalogued as suspected variable star NSV 2008.
1342:
951:, database entry, The Bright Star Catalogue, 5th Revised Ed. (Preliminary Version), D. Hoffleit and W. H. Warren, Jr.,
1819:
502:
2289:
2279:
1814:
1971:
731:
2269:
2274:
2032:
1824:
735:
510:
506:
132:
2192:
2009:
1921:
1803:
796:
615:
518:
494:
402:
83:
2071:
1718:
1637:
1579:
1368:
1317:
1070:
1010:
974:
899:
851:
258:
1478:
514:
1736:
1708:
1627:
1499:
1307:
1088:
1060:
1026:
1000:
867:
841:
691:
522:
279:
115:
1843:
1655:
1595:
1529:
1391:
1333:
1119:
922:
773:
657:
630:
467:
56:
1753:
1109:
551:
1726:
1645:
1587:
1325:
1321:
1078:
1018:
859:
855:
754:
580:
438:
366:
242:
1673:
1871:
1575:
1555:
1411:
788:
379:
187:
91:
1722:
1641:
1583:
1388:
A Dictionary of Modern star Names: A Short Guide to 254 Star Names and Their
Derivations
1372:
1074:
1014:
978:
903:
31:
1901:
1359:
Bernacca, P. L.; Perinotto, M. (1970). "A catalogue of stellar rotational velocities".
804:
768:
758:
498:
485:
250:
230:
218:
2248:
1960:
1896:
1886:
1866:
1861:
1851:
1740:
1731:
1650:
1615:
1115:
1092:
1083:
1030:
743:
687:
683:
679:
611:
207:
78:
871:
2130:
1891:
1876:
750:
339:
309:
1441:
1329:
38:
1462:
863:
1881:
784:
780:
747:
424:
165:
154:
143:
104:
890:
Johnson, H. L.; et al. (1966). "UBVRIJKL photometry of the bright stars".
2138:
2112:
2076:
1999:
1994:
1989:
1954:
1949:
1944:
1939:
1911:
1906:
1591:
1022:
991:
Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation",
956:
832:
van
Leeuwen, F. (November 2007). "Validation of the new Hipparcos reduction".
800:
739:
723:
352:
319:
265:
175:
1659:
1337:
772:. At the distance to this star, it yield a physical radius of 15.9 times the
2104:
1984:
1979:
1934:
1929:
719:
2215:
2210:
2205:
2200:
2055:
2050:
2045:
2040:
2022:
2017:
1772:
715:
474:
2164:
2086:
2081:
66:
59:
2183:
2169:
2156:
1569:
1346:
727:
545:
416:
332:
270:
1674:"Nihal - β Leporis (beta Leporis) - Star in Lepus | TheSkyLive.com"
1312:
1713:
1632:
1114:, Astronomy and astrophysics library, vol. 1 (3rd ed.),
1065:
1005:
846:
1834:
607:
234:
222:
1776:
1758:
New
Catalogue of Suspected Variable Stars, the improved version
637:, Arabic for "quenching their thirst". The occasional spelling
799:, the pair was found to be separated by an angle of 2.58
787:, whereby the second star has a brightness of 7.34 mag. Using
1558:, Hong Kong Space Museum. Accessed on line November 23, 2010.
589:
595:
1500:"Bulletin of the IAU Working Group on Star Names, No. 1"
1390:(2nd rev. ed.). Cambridge, Massachusetts: Sky Pub.
1361:
738:
of G5 II. The mass of this star is 3.5 times the
1614:
Richichi, A.; Percheron, I.; Davis, J. (2009-10-01).
1141:
722:
astrometry satellite, this star is located about 160
586:
493:
Nihal, β Lep, Beta Leporis, Beta Lep,
973:, vol. 30, Academic Press, London, p. 57,
892:
Communications of the Lunar and
Planetary Laboratory
598:
2191:
2182:
2155:
2129:
2103:
2064:
2031:
2008:
1970:
1920:
1842:
1833:
1760:, Moscow, Russia.: Sternberg Astronomical Institute
583:
1274:
1700:Monthly Notices of the Royal Astronomical Society
1620:Monthly Notices of the Royal Astronomical Society
1528:, written by 陳久金. Published by 台灣書房出版有限公司, 2005,
1053:Monthly Notices of the Royal Astronomical Society
1046:
1044:
1042:
1040:
678:, refers to an asterism consisting of β Leporis,
641:appears to be due to a misreading. In 2016, the
16:Second brightest star in the constellation Lepus
923:"CCDM J05283-2046AB -- Double or multiple star"
1467:, New York: G. E. Steichert, pp. 265, 269
827:
825:
823:
821:
819:
1788:
931:Centre de Données astronomiques de Strasbourg
701:
695:
667:
661:
109:−20° 45′ 33.9878″
8:
633:. It is also known by the traditional named
592:
2188:
2152:
2126:
2100:
1839:
1795:
1781:
1773:
1293:
1291:
1289:
1103:
1101:
885:
883:
881:
1730:
1712:
1649:
1631:
1571:The Making of History's Greatest Star Map
1311:
1262:
1233:
1224:
1219:
1206:
1179:
1169:
1156:
1142:
1140:
1082:
1064:
1004:
845:
1479:"IAU Working Group on Star Names (WGSN)"
917:
915:
913:
815:
214:
959:. Accessed on line November 18, 2008.
757:of Beta Leporis, after correction for
18:
1574:, Astronomers' Universe, Heidelberg:
7:
1386:Kunitzsch, Paul; Smart, Tim (2006).
62:
226:
14:
2231:
2230:
1732:10.1111/j.1365-2966.2011.18205.x
1651:10.1111/j.1365-2966.2009.15289.x
1461:Allen, Richard Hinckley (1899),
1084:10.1111/j.1365-2966.2009.15979.x
706:), "the Second Star of Toilet".
643:International Astronomical Union
579:
37:
30:
48:Location of β Leporis (circled)
2285:Henry Draper Catalogue objects
1200:
1172:
1:
2300:Bright Star Catalogue objects
1464:Star-names and Their Meanings
1343:Beta Leporis' database entry
730:) from the Earth. It has an
249:20.34 ± 0.18
1820:List of star names in Lepus
1412:"IAU Catalog of Star Names"
1330:10.1051/0004-6361/201525770
702:
668:
647:Working Group on Star Names
2316:
1815:Lepus in Chinese astronomy
1754:"NSV 2008, database entry"
1568:Perryman, Michael (2010),
1300:Astronomy and Astrophysics
864:10.1051/0004-6361:20078357
834:Astronomy and Astrophysics
606:, is the second brightest
2228:
2151:
2125:
2099:
1810:
1592:10.1007/978-3-642-11602-5
1108:Lang, Kenneth R. (2006),
1023:10.1134/S1063773712050015
732:apparent visual magnitude
696:
662:
538:
491:
484:
480:
303:
298:
294:
181:
174:
126:
53:
24:
694:for β Leporis itself is
2255:Stars with proper names
1322:2015A&A...580A..24D
856:2007A&A...474..653V
280:Absolute magnitude
116:Apparent magnitude
2295:Durchmusterung objects
1825:List of stars in Lepus
1804:Constellation of Lepus
1549:香港太空館 - 研究資源 - 亮星中英對照表
1276:
1111:Astrophysical formulae
736:stellar classification
718:measurements from the
2260:Lepus (constellation)
1277:
797:Haleakala Observatory
2265:G-type bright giants
1139:
783:system and may be a
690:. Consequently, the
1723:2011MNRAS.413.1200R
1642:2009MNRAS.399..399R
1584:2010mhgs.book.....P
1373:1970CoAsi.239....1B
1075:2010MNRAS.402.1369L
1015:2012AstL...38..331A
979:1967IAUS...30...57E
904:1966CoLPL...4...99J
539:Database references
533: 05282-2046A.
447:Rotational velocity
21:
1554:2008-10-25 at the
1272:
1270:
574:), formally named
486:Other designations
229: −85.92
133:Spectral type
19:
2290:Hipparcos objects
2280:Flamsteed objects
2242:
2241:
2224:
2223:
2178:
2177:
2147:
2146:
2121:
2120:
2095:
2094:
1601:978-3-642-11601-8
1534:978-986-7332-25-7
1432:Kaler, James B.,
1397:978-1-931559-44-7
1240:
1222:
1218:
1209:
1205:
993:Astronomy Letters
774:radius of the Sun
631:Bayer designation
560:Beta Leporis
557:
556:
269:(49.2 ± 0.4
217: −5.02
2307:
2234:
2233:
2189:
2153:
2127:
2101:
2072:2MASS J0523−1403
1840:
1797:
1790:
1783:
1774:
1768:
1767:
1766:
1765:
1750:
1744:
1743:
1734:
1716:
1707:(2): 1200–1205,
1694:
1688:
1687:
1685:
1684:
1670:
1664:
1663:
1653:
1635:
1611:
1605:
1604:
1565:
1559:
1547:
1543:
1537:
1524:
1520:
1514:
1513:
1511:
1509:
1504:
1496:
1490:
1489:
1487:
1485:
1475:
1469:
1468:
1458:
1452:
1451:
1450:
1449:
1440:, archived from
1429:
1423:
1422:
1420:
1418:
1408:
1402:
1401:
1383:
1377:
1376:
1356:
1350:
1341:
1315:
1295:
1284:
1281:
1279:
1278:
1273:
1271:
1267:
1266:
1245:
1241:
1239:
1238:
1237:
1228:
1223:
1220:
1216:
1211:
1210:
1207:
1203:
1187:
1186:
1170:
1161:
1160:
1128:
1105:
1096:
1095:
1086:
1068:
1059:(2): 1369–1379,
1048:
1035:
1034:
1008:
988:
982:
981:
966:
960:
946:
940:
939:
938:
937:
919:
908:
907:
887:
876:
875:
849:
829:
771:
766:
755:angular diameter
705:
699:
698:
671:
665:
664:
605:
604:
601:
600:
597:
594:
591:
588:
585:
436:
434:
414:
412:
392:
364:
362:
317:
228:
216:
200:
127:Characteristics
119:
99:
94:
54:Observation data
41:
34:
22:
2315:
2314:
2310:
2309:
2308:
2306:
2305:
2304:
2245:
2244:
2243:
2238:
2220:
2174:
2143:
2117:
2091:
2060:
2027:
2004:
1966:
1916:
1829:
1806:
1801:
1771:
1763:
1761:
1752:
1751:
1747:
1696:
1695:
1691:
1682:
1680:
1672:
1671:
1667:
1613:
1612:
1608:
1602:
1576:Springer-Verlag
1567:
1566:
1562:
1556:Wayback Machine
1545:
1544:
1540:
1522:
1521:
1517:
1507:
1505:
1502:
1498:
1497:
1493:
1483:
1481:
1477:
1476:
1472:
1460:
1459:
1455:
1447:
1445:
1431:
1430:
1426:
1416:
1414:
1410:
1409:
1405:
1398:
1385:
1384:
1380:
1358:
1357:
1353:
1297:
1296:
1287:
1269:
1268:
1258:
1243:
1242:
1229:
1212:
1175:
1171:
1162:
1152:
1137:
1136:
1133:) is given by:
1132:
1129:. The radius (R
1126:
1107:
1106:
1099:
1050:
1049:
1038:
990:
989:
985:
968:
967:
963:
947:
943:
935:
933:
921:
920:
911:
889:
888:
879:
831:
830:
817:
813:
789:adaptive optics
764:
762:
740:mass of the Sun
712:
653:for this star.
624:
582:
578:
534:
501:−20 1096,
497:, 9 Lep,
453: sin
432:
430:
410:
408:
390:
380:Surface gravity
372:
369:
360:
358:
345:
342:
325:
322:
315:
285:
268:
225:
198:
193:
188:Radial velocity
114:
97:
92:Right ascension
90:
55:
49:
47:
46:
45:
44:
43:
42:
17:
12:
11:
5:
2313:
2311:
2303:
2302:
2297:
2292:
2287:
2282:
2277:
2272:
2270:Multiple stars
2267:
2262:
2257:
2247:
2246:
2240:
2239:
2229:
2226:
2225:
2222:
2221:
2219:
2218:
2213:
2208:
2203:
2197:
2195:
2186:
2180:
2179:
2176:
2175:
2173:
2172:
2167:
2161:
2159:
2149:
2148:
2145:
2144:
2142:
2141:
2135:
2133:
2123:
2122:
2119:
2118:
2116:
2115:
2109:
2107:
2097:
2096:
2093:
2092:
2090:
2089:
2084:
2079:
2074:
2068:
2066:
2062:
2061:
2059:
2058:
2053:
2048:
2043:
2037:
2035:
2029:
2028:
2026:
2025:
2020:
2014:
2012:
2006:
2005:
2003:
2002:
1997:
1992:
1987:
1982:
1976:
1974:
1968:
1967:
1965:
1964:
1957:
1952:
1947:
1942:
1937:
1932:
1926:
1924:
1918:
1917:
1915:
1914:
1909:
1904:
1899:
1894:
1889:
1884:
1879:
1874:
1869:
1864:
1859:
1854:
1848:
1846:
1837:
1831:
1830:
1828:
1827:
1822:
1817:
1811:
1808:
1807:
1802:
1800:
1799:
1792:
1785:
1777:
1770:
1769:
1745:
1689:
1678:theskylive.com
1665:
1626:(1): 399–409.
1606:
1600:
1560:
1538:
1515:
1491:
1470:
1453:
1424:
1403:
1396:
1378:
1351:
1285:
1283:
1282:
1265:
1261:
1257:
1254:
1251:
1248:
1246:
1244:
1236:
1232:
1227:
1215:
1202:
1199:
1196:
1193:
1190:
1185:
1182:
1178:
1174:
1168:
1165:
1163:
1159:
1155:
1151:
1148:
1145:
1144:
1130:
1124:
1097:
1036:
983:
961:
941:
909:
877:
840:(2): 653–664.
814:
812:
809:
805:position angle
793:AEOS telescope
759:limb darkening
734:of 2.84 and a
711:
708:
629:is the star's
623:
620:
566:, abbreviated
564:β Leporis
555:
554:
549:
541:
540:
536:
535:
529: 170457,
525: 248938,
495:9 Leporis
492:
489:
488:
482:
481:
478:
477:
471:
463:
462:
459:
442:
441:
428:
420:
419:
406:
398:
397:
388:
375:
374:
370:
367:
356:
348:
347:
343:
340:
336:
328:
327:
323:
320:
313:
305:
304:
301:
300:
296:
295:
292:
291:
288:
283:
275:
274:
262:
254:
253:
247:
238:
237:
212:
203:
202:
196:
191:
183:
182:
179:
178:
172:
171:
168:
161:
160:
157:
150:
149:
146:
139:
138:
135:
129:
128:
124:
123:
120:
111:
110:
107:
101:
100:
98:05 28 14.72316
95:
87:
86:
81:
75:
74:
51:
50:
36:
35:
29:
28:
27:
26:
25:
15:
13:
10:
9:
6:
4:
3:
2:
2312:
2301:
2298:
2296:
2293:
2291:
2288:
2286:
2283:
2281:
2278:
2276:
2275:Bayer objects
2273:
2271:
2268:
2266:
2263:
2261:
2258:
2256:
2253:
2252:
2250:
2237:
2227:
2217:
2214:
2212:
2209:
2207:
2204:
2202:
2199:
2198:
2196:
2194:
2190:
2187:
2185:
2181:
2171:
2168:
2166:
2163:
2162:
2160:
2158:
2154:
2150:
2140:
2137:
2136:
2134:
2132:
2131:Star clusters
2128:
2124:
2114:
2111:
2110:
2108:
2106:
2102:
2098:
2088:
2085:
2083:
2080:
2078:
2075:
2073:
2070:
2069:
2067:
2063:
2057:
2054:
2052:
2049:
2047:
2044:
2042:
2039:
2038:
2036:
2034:
2030:
2024:
2021:
2019:
2016:
2015:
2013:
2011:
2007:
2001:
1998:
1996:
1993:
1991:
1988:
1986:
1983:
1981:
1978:
1977:
1975:
1973:
1969:
1963:
1962:
1958:
1956:
1953:
1951:
1948:
1946:
1943:
1941:
1938:
1936:
1933:
1931:
1928:
1927:
1925:
1923:
1919:
1913:
1910:
1908:
1905:
1903:
1900:
1898:
1895:
1893:
1890:
1888:
1885:
1883:
1880:
1878:
1875:
1873:
1870:
1868:
1865:
1863:
1860:
1858:
1855:
1853:
1850:
1849:
1847:
1845:
1841:
1838:
1836:
1832:
1826:
1823:
1821:
1818:
1816:
1813:
1812:
1809:
1805:
1798:
1793:
1791:
1786:
1784:
1779:
1778:
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1444:on 2008-12-10
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1125:3-540-29692-1
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749:
746:, becoming a
745:
744:main sequence
741:
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733:
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709:
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693:
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636:
632:
628:
621:
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617:
613:
612:constellation
609:
603:
577:
573:
569:
568:Beta Lep
565:
561:
553:
550:
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543:
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537:
532:
528:
524:
520:
517: 25606,
516:
513: 36079,
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267:
264:160 ± 1
263:
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246:
244:
240:
239:
236:
232:
224:
220:
213:
211:
209:
208:Proper motion
205:
204:
197:
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96:
93:
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79:Constellation
77:
76:
72:
68:
65:
61:
58:
52:
40:
33:
23:
1959:
1856:
1762:, retrieved
1757:
1748:
1704:
1698:
1692:
1681:. Retrieved
1677:
1668:
1623:
1619:
1609:
1570:
1563:
1546:(in Chinese)
1541:
1525:
1523:(in Chinese)
1518:
1506:. Retrieved
1494:
1482:. Retrieved
1473:
1463:
1456:
1446:, retrieved
1442:the original
1437:
1427:
1415:. Retrieved
1406:
1387:
1381:
1364:
1360:
1354:
1303:
1299:
1110:
1056:
1052:
996:
992:
986:
970:
964:
944:
934:, retrieved
926:
895:
891:
837:
833:
778:
751:bright giant
713:
692:Chinese name
673:
655:
650:
645:organized a
638:
634:
627:Beta Leporis
626:
625:
622:Nomenclature
575:
571:
567:
563:
559:
558:
544:
521: 1829,
509: 6762,
466:
461:11 km/s
454:
450:
445:
423:
401:
383:
378:
351:
331:
308:
278:
257:
241:
206:
186:
781:double star
767:0.066
724:light-years
672:), meaning
505: 204,
425:Metallicity
403:Temperature
391:2.60 ± 0.03
199:−13.6 ± 0.9
166:color index
155:color index
144:color index
137:G5 II
105:Declination
2249:Categories
2139:Messier 79
2113:HD 33283 b
2105:Exoplanets
2077:Gliese 229
1764:2008-11-18
1683:2023-03-28
1448:2008-11-18
1313:1505.01726
1116:Birkhäuser
999:(5): 331,
936:2011-12-27
898:(99): 99.
811:References
801:arcseconds
779:This is a
710:Properties
572:β Lep
382:(log
353:Luminosity
338:15.9
201: km/s
176:Astrometry
20:β Leporis
1922:Flamsteed
1857:β (Nihal)
1852:α (Arneb)
1741:118398949
1714:1012.3383
1660:0035-8711
1633:0906.3981
1338:0004-6361
1264:⨀
1256:⋅
1250:≈
1235:⨀
1214:0.0046491
1195:⋅
1189:⋅
1181:−
1158:∗
1150:⋅
1093:119096173
1066:0911.1335
1031:119257644
1006:1108.4971
847:0708.1752
720:Hipparcos
714:Based on
688:δ Leporis
684:γ Leporis
680:α Leporis
473:240
316:3.5 ± 0.1
118: (V)
2236:Category
2184:Galaxies
1972:Variable
1552:Archived
1367:(1): 1.
872:18759600
716:parallax
371:☉
344:☉
324:☉
282: (M
259:Distance
243:Parallax
2165:Abell 7
2157:Nebulae
2087:WASP-61
2082:WASP-49
1719:Bibcode
1638:Bibcode
1580:Bibcode
1508:28 July
1434:"Nihal"
1417:28 July
1369:Bibcode
1318:Bibcode
1306:: A24.
1071:Bibcode
1011:Bibcode
975:Bibcode
949:HR 1829
900:Bibcode
852:Bibcode
791:on the
728:parsecs
658:Chinese
610:in the
299:Details
67:J2000.0
64:Equinox
60:J2000.0
2170:IC 418
1739:
1658:
1598:
1532:
1526:中國星座神話
1484:22 May
1394:
1347:VizieR
1336:
1217:
1204:
1122:
1091:
1029:
927:SIMBAD
870:
785:binary
753:. The
748:G-type
675:Toilet
546:SIMBAD
437:
415:
393:
365:
333:Radius
318:
170:+0.44
159:+0.82
148:+0.47
2065:Other
2056:33283
2051:33142
2046:32450
2041:31527
1961:4 Mon
1844:Bayer
1835:Stars
1737:S2CID
1709:arXiv
1628:arXiv
1503:(PDF)
1438:Stars
1308:arXiv
1253:31.78
1198:3.003
1089:S2CID
1061:arXiv
1027:S2CID
1001:arXiv
868:S2CID
842:arXiv
803:at a
763:3.003
761:, is
703:Cè èr
651:Nihal
639:Nibal
635:Nihal
616:Lepus
576:Nihal
431:−0.12
409:5,434
290:−0.65
227:Dec.:
122:2.84
84:Lepus
57:Epoch
2216:2139
2211:1993
2206:1979
2201:1964
2023:1762
2018:1621
1656:ISSN
1596:ISBN
1530:ISBN
1510:2016
1486:2016
1419:2016
1392:ISBN
1334:ISSN
1192:49.2
1120:ISBN
957:V/50
726:(49
686:and
608:star
552:data
435:0.06
310:Mass
164:R−I
153:B−V
142:U−B
71:ICRS
2193:NGC
1727:doi
1705:413
1646:doi
1624:399
1588:doi
1365:239
1345:at
1326:doi
1304:580
1079:doi
1057:402
1019:doi
955:ID
953:CDS
860:doi
838:474
795:at
769:mas
656:In
614:of
531:WDS
527:SAO
523:PPM
515:HIP
503:FK5
475:Myr
468:Age
439:dex
395:cgs
359:160
251:mas
245:(π)
231:mas
219:mas
215:RA:
210:(μ)
2251::
2033:HD
2010:HR
2000:AK
1995:AF
1990:RX
1955:19
1950:17
1945:12
1940:10
1756:,
1735:,
1725:,
1717:,
1703:,
1676:.
1654:.
1644:.
1636:.
1622:.
1618:.
1594:,
1586:,
1578:,
1436:,
1363:.
1332:.
1324:.
1316:.
1302:.
1288:^
1221:AU
1208:AU
1177:10
1118:,
1100:^
1087:,
1077:,
1069:,
1055:,
1039:^
1025:,
1017:,
1009:,
997:38
995:,
929:,
925:,
912:^
894:.
880:^
866:.
858:.
850:.
836:.
818:^
776:.
697:廁二
682:,
669:Cè
660:,
618:.
590:aɪ
570:,
519:HR
511:HD
507:GC
499:BD
413:38
271:pc
266:ly
235:yr
223:yr
190:(R
73:)
1985:T
1980:R
1935:8
1930:1
1912:ν
1907:μ
1902:λ
1897:κ
1892:ι
1887:θ
1882:η
1877:ζ
1872:ε
1867:δ
1862:γ
1796:e
1789:t
1782:v
1729::
1721::
1711::
1686:.
1662:.
1648::
1640::
1630::
1590::
1582::
1536:.
1512:.
1488:.
1421:.
1400:.
1375:.
1371::
1349:.
1340:.
1328::
1320::
1310::
1260:R
1231:R
1226:/
1201:)
1184:3
1173:(
1167:=
1154:R
1147:2
1131:*
1081::
1073::
1063::
1033:.
1021::
1013::
1003::
977::
906:.
902::
896:4
874:.
862::
854::
844::
765:±
700:(
666:(
663:廁
602:/
599:l
596:æ
593:.
587:n
584:ˈ
581:/
562:(
457:)
455:i
451:v
449:(
433:±
417:K
411:±
386:)
384:g
368:L
363:3
361:±
341:R
321:M
286:)
284:V
273:)
233:/
221:/
194:)
192:v
69:(
Text is available under the Creative Commons Attribution-ShareAlike License. Additional terms may apply.
