Knowledge

Barred spiral galaxy

Source đź“ť

360: 186: 667: 31: 579: 443: 170:
Simulations show that many bars likely experience a "buckling" event in which a disturbance in the orbital resonances of stars in the bar structure leads to an inward collapse in which the bar becomes thicker and shorter though the exact mechanism behind this buckling instability remains hotly debated. Barred spiral galaxies with high mass accumulated in their center thus tend to have short, stubby bars. Such buckling phenomena are significantly suppressed and delayed by the presence of a
601: 205: 284: 119: 2412: 341: 2424: 623: 322: 2464: 303: 398: 2488: 645: 2476: 535: 513: 693: 2452: 715: 261: 417: 379: 491: 979:
Costantin, Luca; Pérez-González, Pablo G.; Guo, Yuchen; Buttitta, Chiara; Jogee, Shardha; Bagley, Micaela B.; Barro, Guillermo; Kartaltepe, Jeyhan S.; Koekemoer, Anton M.; Cabello, Cristina; Corsini, Enrico Maria; Méndez-Abreu, Jairo; de la Vega, Alexander; Iyer, Kartheik G.; Bisigello, Laura (2023).
219:
The general classification is "SB" (spiral barred). The sub-categories are based on how open or tight the arms of the spiral are. SBa types feature tightly bound arms. SBc types are at the other extreme and have loosely bound arms. SBb galaxies lie in between. SBm describes somewhat irregular barred
169:
Bars are thought to be temporary phenomena in the lives of spiral galaxies; the bar structures decay over time, transforming galaxies from barred spirals to more "regular" spiral patterns. Past a certain size the accumulated mass of the bar compromises the stability of the overall bar structure.
181:
Recent studies have confirmed the idea that bars are a sign of galaxies reaching full maturity as the "formative years" end. A 2008 investigation found that only 20 percent of the spiral galaxies in the distant past possessed bars, compared with about 65 percent of their local counterparts.
1055:
Guo, Yuchen; Jogee, Shardha; Finkelstein, Steven L.; Chen, Zilei; Wise, Eden; Bagley, Micaela B.; Barro, Guillermo; Wuyts, Stijn; Kocevski, Dale D.; Kartaltepe, Jeyhan S.; McGrath, Elizabeth J.; Ferguson, Henry C.; Mobasher, Bahram; Giavalisco, Mauro; Lucas, Ray A. (2023-03-01).
103:
Although theoretical models of galaxy formation and evolution had not previously expected galaxies becoming stable enough to host bars very early in the universe's history, evidence has recently emerged of the existence of numerous spiral galaxies in the early universe.
177:
Since so many spiral galaxies have bar structures, it is likely that they are recurring phenomena in spiral galaxy development. The oscillating evolutionary cycle from spiral galaxy to barred spiral galaxy is thought to take on average about two billion years.
557: 83:
and arranged them into sub-categories based on how open the arms of the spiral are. SBa types feature tightly bound arms, while SBc types are at the other extreme and have loosely bound arms. SBb-type galaxies lie in between the two. SB0 is a barred
138:
radiating from the center of the galaxy whose effects reshape the orbits of the inner stars. This effect builds over time to stars orbiting farther out, which creates a self-perpetuating bar structure.
96:, which were once classified as irregular galaxies, but have since been found to contain barred spiral structures. Among other types in Hubble's classifications for the galaxies are the spiral galaxy, 1395: 134:
Barred galaxies are apparently predominant, with surveys showing that up to two-thirds of all spiral galaxies develop a bar. The creation of the bar is generally thought to be the result of a
1416:
Sheth, Kartik; Elmegreen, Debra Meloy; Elmegreen, Bruce G.; et al. (2008). "Evolution of the Bar Fraction in COSMOS: Quantifying the Assembly of the Hubble Sequence".
2234: 2281: 1392: 1931: 1619: 359: 1592: 1317: 899: 870: 1580:, 1995. "Astronomers Find Multiple Generations of Star Formation in Central Starburst Ring of a Barred Spiral Galaxy." January 15, 2000. 2523: 1664: 737: 472: 238: 191: 2347: 2266: 57:. Bars are found in about two thirds of all spiral galaxies in the local universe, and generally affect both the motions of stars and 1647: 2508: 666: 185: 1485: 2352: 1562: 742: 2079: 1610: 1123: 2249: 1515: 1577: 1334:
Wheeler, Vance; Valluri, Monica; Silva, Leandro Beraldo e; Dattathri, Shashank; Debattista, Victor P. (2023-11-16).
2442: 2367: 2322: 2130: 1719: 1714: 1687: 723: 578: 30: 2048: 1555: 212: 2518: 2513: 2332: 2244: 2239: 2145: 2041: 1999: 1709: 1682: 587: 425: 221: 163: 2327: 2312: 2259: 1918: 1906: 1901: 1815: 1780: 1751: 1741: 701: 594: 171: 158:
in the vicinity of its center. This process is also thought to explain why many barred spiral galaxies have
89: 1830: 1729: 967: 638: 616: 609: 572: 159: 38: 2357: 2254: 1956: 499: 442: 2387: 2337: 2172: 2084: 1640: 1435: 1357: 1276: 1221: 1164: 1079: 1003: 934: 823: 767: 2492: 2150: 2058: 1989: 1881: 1756: 1403: 891: 600: 543: 135: 113: 2423: 204: 2480: 2468: 2382: 2377: 2362: 2317: 2286: 2271: 2189: 2157: 1994: 1946: 1936: 1459: 1425: 1347: 1300: 1266: 1239: 1211: 1180: 1154: 1069: 993: 950: 924: 839: 550: 1596: 2415: 2397: 2372: 2342: 2221: 2063: 2053: 2036: 1968: 1797: 1763: 1724: 1677: 1540: 1451: 1375: 1321: 1292: 1145:
F. Bournaud; F. Combes (2002). "Gas accretion on spiral galaxies: Bar formation and renewal".
1097: 1037: 1019: 895: 866: 787: 762: 757: 660: 528: 506: 484: 449: 267: 155: 151: 97: 93: 85: 814:
P. B. Eskridge; J. A. Frogel (1999). "What is the True Fraction of Barred Spiral Galaxies?".
2427: 2229: 2204: 2184: 2179: 2167: 2021: 1842: 1775: 1443: 1365: 1284: 1280: 1229: 1172: 1168: 1087: 1027: 1011: 942: 831: 827: 147: 127: 66: 58: 1058:"First Look at z > 1 Bars in the Rest-frame Near-infrared with JWST Early CEERS Imaging" 283: 2276: 2199: 1891: 1864: 1835: 1787: 1633: 1399: 143: 118: 80: 1439: 1361: 1225: 1083: 1032: 1007: 981: 938: 2140: 1973: 1876: 1871: 1825: 1768: 521: 2502: 2296: 2162: 2125: 1896: 1859: 1847: 1699: 1694: 1584: 1304: 1234: 1199: 862: 843: 477: 50: 1603: 1463: 1243: 1184: 954: 17: 2456: 2291: 2194: 2135: 2120: 2026: 1951: 1746: 1736: 1477: 1115: 340: 76: 70: 1288: 1200:"Circumnuclear regions in barred spiral galaxies - II. Relations to host galaxies" 556: 1176: 2392: 2209: 2099: 2089: 1886: 1852: 1792: 1672: 653: 622: 369: 321: 1507: 1370: 1336:"Early-growing Supermassive Black Holes Strengthen Bars and Boxy/Peanut Bulges" 1335: 1092: 1057: 1015: 2094: 2031: 946: 835: 565: 312: 302: 62: 1455: 1379: 1296: 1101: 1023: 2104: 686: 397: 126:, located more than 40 million light-years from Earth. It was discovered by 1604:"ESO Provides An Infrared Portrait of the Barred Spiral Galaxy Messier 83." 1041: 644: 1216: 1159: 929: 708: 407: 388: 350: 331: 293: 274: 251: 208: 34: 416: 79:
classified spiral galaxies of this type as "SB" (spiral, barred) in his
752: 747: 534: 378: 123: 692: 512: 1941: 1926: 1656: 679: 675: 631: 433: 714: 260: 2451: 1447: 1352: 1271: 1074: 998: 27:
Spiral galaxy with a central bar-shaped structure composed of stars
2014: 2009: 2004: 1961: 1549:
An article about the Spitzer Space Telescope's Milky Way discovery
1430: 1257:
Lokas, Ewa L. (2019-09-06). "Anatomy of a buckling galactic bar".
203: 184: 117: 29: 1561:
The original press release regarding the article above, from the
88:. A new type, SBm, was subsequently created to describe somewhat 54: 1629: 490: 1625: 915:
Gerhard, Ortwin (2002). "Mass distribution in our Galaxy".
982:"A Milky Way-like barred spiral galaxy at a redshift of 3" 1620:"Spitzer NGC 1291 barred spiral galaxy seen in infrared." 1570: 1543: 1541:"Milky Way’s Central Structure Seen with Fresh Clarity." 462: 231: 1556:"Galactic survey reveals a new look for the Milky Way." 1569:'Barred' Spiral Galaxy Pic Highlights Stellar Birth." 2440: 73:
is located, is classified as a barred spiral galaxy.
888:
The Whole Shebang: A State-of-the-Universe(s) Report
2305: 2220: 2113: 2072: 1982: 1917: 1808: 1663: 142:The bar structure is believed to act as a type of 1204:Monthly Notices of the Royal Astronomical Society 1198:J. H. Knapen; D. PĂ©rez-RamĂ­rez; S. Laine (2002). 968:Milky Way-like galaxy found in the early universe 53:with a central bar-shaped structure composed of 114:Density wave theory § Galactic spiral arms 174:in the galactic center but occur nonetheless. 2282:List of the most distant astronomical objects 1641: 8: 1648: 1634: 1626: 809: 807: 259: 1429: 1369: 1351: 1270: 1233: 1215: 1158: 1091: 1073: 1031: 997: 928: 190:Milky Way Galaxy spiral arms - based on 2447: 779: 61:within spiral galaxies and can affect 1126:from the original on 15 December 2016 150:inwards from the spiral arms through 7: 1578:Classifying Galaxies: Barred Spirals 1576:Hastings, George and Jane Hastings. 1488:from the original on 7 February 2017 738:Galaxy morphological classification 422:SBdm can also be considered a type 25: 1062:The Astrophysical Journal Letters 211:is a barred spiral galaxy in the 2486: 2474: 2462: 2450: 2422: 2411: 2410: 1235:10.1046/j.1365-8711.2002.05840.x 713: 691: 665: 643: 621: 599: 577: 555: 533: 511: 489: 441: 415: 396: 377: 358: 339: 320: 301: 282: 1518:from the original on 2017-09-22 2353:Galaxy formation and evolution 2348:Galaxy color–magnitude diagram 816:Astrophysics and Space Science 743:Galaxy formation and evolution 1: 1611:European Southern Observatory 1508:"Galactic David and Goliath" 1259:Astronomy & Astrophysics 2235:Galaxies named after people 1289:10.1051/0004-6361/201936056 162:, such as that seen in the 2540: 2524:Galaxy morphological types 2368:Gravitational microlensing 2323:Galactic coordinate system 1593:Barred spirals come and go 1393:Ripples in a Galactic Pond 1318:Barred Spirals Come and Go 1177:10.1051/0004-6361:20020920 1147:Astronomy and Astrophysics 1116:"A closer look at IC 5201" 1016:10.1038/s41586-023-06636-x 111: 2406: 1609:A press release from the 1418:The Astrophysical Journal 1340:The Astrophysical Journal 37:, viewed nearly face-on; 2333:Galactic magnetic fields 2146:Brightest cluster galaxy 2042:Luminous infrared galaxy 1371:10.3847/1538-4357/ace962 1093:10.3847/2041-8213/acacfb 426:barred Magellanic spiral 222:barred lenticular galaxy 164:Southern Pinwheel Galaxy 90:irregular barred spirals 2328:Galactic habitable zone 2313:Extragalactic astronomy 1902:Supermassive black hole 1816:Active galactic nucleus 1478:"A spiral in Andromeda" 1281:2019A&A...629A..52L 1169:2002A&A...392...83B 947:10.1023/A:1015818111633 886:Timothy Ferris (1998). 836:10.1023/A:1017025820201 828:1999Ap&SS.269..427E 172:supermassive black hole 2509:Barred spiral galaxies 2080:Low surface brightness 1831:Central massive object 1512:www.spacetelescope.org 1482:www.spacetelescope.org 1120:www.spacetelescope.org 788:"Barred spiral galaxy" 216: 196: 160:active galactic nuclei 131: 100:and irregular galaxy. 42: 39:Hubble Space Telescope 2358:Galaxy rotation curve 917:Space Science Reviews 207: 188: 122:Barred spiral galaxy 121: 112:Further information: 33: 2393:Population III stars 2388:Intergalactic travel 2338:Galactic orientation 2205:Voids and supervoids 892:Simon & Schuster 768:Firehose instability 47:barred spiral galaxy 18:Barred Spiral galaxy 2383:Intergalactic stars 2272:Large quasar groups 2267:Groups and clusters 2131:Groups and clusters 1990:Lyman-alpha emitter 1882:Interstellar medium 1606:November 29, 2001. 1597:Sky & Telescope 1587:concerning NGC 1326 1539:Britt, Robert Roy. 1440:2008ApJ...675.1141S 1404:Scientific American 1362:2023ApJ...958..119W 1226:2002MNRAS.337..808K 1084:2023ApJ...945L..10G 1008:2023Natur.623..499C 939:2002SSRv..100..129G 857:D. Mihalas (1968). 2378:Intergalactic dust 2363:Gravitational lens 2318:Galactic astronomy 2287:Starburst galaxies 2027:blue compact dwarf 1983:Energetic galaxies 1947:BL Lacertae object 1563:Univ. of Wisconsin 1398:2007-09-28 at the 859:Galactic Astronomy 220:spirals. SB0 is a 217: 197: 132: 43: 2438: 2437: 2398:Galaxy X (galaxy) 2373:Illustris project 2343:Galactic quadrant 2064:Wolf-Rayet galaxy 2054:Green bean galaxy 2049:Hot dust-obscured 2000:Luminous infrared 1764:Elliptical galaxy 1322:Sky and Telescope 992:(7987): 499–501. 901:978-0-6848-3861-8 872:978-0-7167-0326-6 763:Lenticular galaxy 758:Ceers-2112 galaxy 729: 728: 661:Magellanic Clouds 456: 455: 450:Magellanic spiral 448:SBm is a type of 268:lenticular galaxy 266:SB0 is a type of 152:orbital resonance 98:elliptical galaxy 94:Magellanic Clouds 86:lenticular galaxy 16:(Redirected from 2531: 2491: 2490: 2489: 2479: 2478: 2477: 2467: 2466: 2465: 2455: 2454: 2446: 2426: 2414: 2413: 2059:Hanny's Voorwerp 1969:Relativistic jet 1843:Dark matter halo 1650: 1643: 1636: 1627: 1622:22 October 2014. 1558:16 August 2005. 1546:16 August 2005. 1527: 1526: 1524: 1523: 1504: 1498: 1497: 1495: 1493: 1474: 1468: 1467: 1433: 1424:(2): 1141–1155. 1413: 1407: 1390: 1384: 1383: 1373: 1355: 1331: 1325: 1315: 1309: 1308: 1274: 1254: 1248: 1247: 1237: 1219: 1217:astro-ph/0207258 1195: 1189: 1188: 1162: 1160:astro-ph/0206273 1142: 1136: 1135: 1133: 1131: 1112: 1106: 1105: 1095: 1077: 1052: 1046: 1045: 1035: 1001: 976: 970: 965: 959: 958: 932: 930:astro-ph/0203110 912: 906: 905: 883: 877: 876: 854: 848: 847: 811: 802: 801: 799: 798: 784: 717: 695: 669: 647: 625: 603: 581: 559: 537: 515: 493: 463: 445: 419: 400: 381: 362: 343: 324: 305: 286: 263: 232: 67:Milky Way Galaxy 59:interstellar gas 21: 2539: 2538: 2534: 2533: 2532: 2530: 2529: 2528: 2519:Barred galaxies 2514:Spiral galaxies 2499: 2498: 2497: 2487: 2485: 2475: 2473: 2463: 2461: 2449: 2441: 2439: 2434: 2402: 2301: 2216: 2109: 2068: 1978: 1913: 1892:Galaxy filament 1836:Galactic Center 1804: 1659: 1654: 1618:Horton, Adam. 1554:Devitt, Terry. 1536: 1531: 1530: 1521: 1519: 1506: 1505: 1501: 1491: 1489: 1476: 1475: 1471: 1415: 1414: 1410: 1400:Wayback Machine 1391: 1387: 1333: 1332: 1328: 1316: 1312: 1256: 1255: 1251: 1197: 1196: 1192: 1144: 1143: 1139: 1129: 1127: 1114: 1113: 1109: 1054: 1053: 1049: 978: 977: 973: 966: 962: 914: 913: 909: 902: 885: 884: 880: 873: 856: 855: 851: 813: 812: 805: 796: 794: 786: 785: 781: 776: 734: 461: 230: 202: 195: 144:stellar nursery 116: 110: 81:Hubble sequence 28: 23: 22: 15: 12: 11: 5: 2537: 2535: 2527: 2526: 2521: 2516: 2511: 2501: 2500: 2496: 2495: 2483: 2471: 2459: 2436: 2435: 2433: 2432: 2420: 2407: 2404: 2403: 2401: 2400: 2395: 2390: 2385: 2380: 2375: 2370: 2365: 2360: 2355: 2350: 2345: 2340: 2335: 2330: 2325: 2320: 2315: 2309: 2307: 2303: 2302: 2300: 2299: 2294: 2289: 2284: 2279: 2274: 2269: 2264: 2263: 2262: 2257: 2252: 2247: 2242: 2237: 2226: 2224: 2218: 2217: 2215: 2214: 2213: 2212: 2202: 2197: 2192: 2190:Stellar stream 2187: 2182: 2177: 2176: 2175: 2170: 2165: 2155: 2154: 2153: 2148: 2143: 2138: 2128: 2123: 2117: 2115: 2111: 2110: 2108: 2107: 2102: 2097: 2092: 2087: 2082: 2076: 2074: 2070: 2069: 2067: 2066: 2061: 2056: 2051: 2046: 2045: 2044: 2039: 2034: 2029: 2019: 2018: 2017: 2012: 2007: 1997: 1992: 1986: 1984: 1980: 1979: 1977: 1976: 1971: 1966: 1965: 1964: 1959: 1949: 1944: 1939: 1934: 1929: 1923: 1921: 1915: 1914: 1912: 1911: 1910: 1909: 1899: 1894: 1889: 1884: 1879: 1877:Galactic ridge 1874: 1872:Galactic plane 1869: 1868: 1867: 1857: 1856: 1855: 1845: 1840: 1839: 1838: 1828: 1823: 1818: 1812: 1810: 1806: 1805: 1803: 1802: 1801: 1800: 1790: 1785: 1784: 1783: 1773: 1772: 1771: 1761: 1760: 1759: 1754: 1749: 1744: 1734: 1733: 1732: 1727: 1722: 1717: 1712: 1707: 1702: 1692: 1691: 1690: 1685: 1675: 1669: 1667: 1661: 1660: 1655: 1653: 1652: 1645: 1638: 1630: 1624: 1623: 1616: 1615: 1614: 1601: 1590: 1589: 1588: 1574: 1567: 1566: 1565: 1552: 1551: 1550: 1535: 1534:External links 1532: 1529: 1528: 1499: 1469: 1448:10.1086/524980 1408: 1406:, October 2005 1385: 1326: 1310: 1249: 1210:(3): 808–828. 1190: 1137: 1107: 1047: 971: 960: 907: 900: 878: 871: 849: 803: 778: 777: 775: 772: 771: 770: 765: 760: 755: 750: 745: 740: 733: 730: 727: 726: 721: 718: 711: 705: 704: 699: 696: 689: 683: 682: 673: 670: 663: 657: 656: 651: 648: 641: 635: 634: 629: 626: 619: 613: 612: 607: 604: 597: 591: 590: 585: 582: 575: 569: 568: 563: 560: 553: 547: 546: 541: 538: 531: 525: 524: 522:Coma Berenices 519: 516: 509: 503: 502: 497: 494: 487: 481: 480: 475: 470: 467: 460: 459:Other examples 457: 454: 453: 446: 439: 436: 430: 429: 420: 413: 410: 404: 403: 401: 394: 391: 385: 384: 382: 375: 372: 366: 365: 363: 356: 353: 347: 346: 344: 337: 334: 328: 327: 325: 318: 315: 309: 308: 306: 299: 296: 290: 289: 287: 280: 277: 271: 270: 264: 257: 254: 248: 247: 244: 241: 236: 229: 226: 215:constellation. 201: 198: 189: 109: 106: 92:, such as the 26: 24: 14: 13: 10: 9: 6: 4: 3: 2: 2536: 2525: 2522: 2520: 2517: 2515: 2512: 2510: 2507: 2506: 2504: 2494: 2484: 2482: 2472: 2470: 2460: 2458: 2453: 2448: 2444: 2431: 2430: 2425: 2421: 2419: 2418: 2409: 2408: 2405: 2399: 2396: 2394: 2391: 2389: 2386: 2384: 2381: 2379: 2376: 2374: 2371: 2369: 2366: 2364: 2361: 2359: 2356: 2354: 2351: 2349: 2346: 2344: 2341: 2339: 2336: 2334: 2331: 2329: 2326: 2324: 2321: 2319: 2316: 2314: 2311: 2310: 2308: 2304: 2298: 2295: 2293: 2292:Superclusters 2290: 2288: 2285: 2283: 2280: 2278: 2275: 2273: 2270: 2268: 2265: 2261: 2258: 2256: 2253: 2251: 2248: 2246: 2243: 2241: 2238: 2236: 2233: 2232: 2231: 2228: 2227: 2225: 2223: 2219: 2211: 2208: 2207: 2206: 2203: 2201: 2198: 2196: 2195:Superclusters 2193: 2191: 2188: 2186: 2183: 2181: 2178: 2174: 2171: 2169: 2166: 2164: 2161: 2160: 2159: 2156: 2152: 2149: 2147: 2144: 2142: 2139: 2137: 2134: 2133: 2132: 2129: 2127: 2126:Galactic tide 2124: 2122: 2119: 2118: 2116: 2112: 2106: 2103: 2101: 2098: 2096: 2093: 2091: 2088: 2086: 2085:Ultra diffuse 2083: 2081: 2078: 2077: 2075: 2071: 2065: 2062: 2060: 2057: 2055: 2052: 2050: 2047: 2043: 2040: 2038: 2035: 2033: 2030: 2028: 2025: 2024: 2023: 2020: 2016: 2013: 2011: 2008: 2006: 2003: 2002: 2001: 1998: 1996: 1993: 1991: 1988: 1987: 1985: 1981: 1975: 1972: 1970: 1967: 1963: 1960: 1958: 1955: 1954: 1953: 1950: 1948: 1945: 1943: 1940: 1938: 1935: 1933: 1930: 1928: 1925: 1924: 1922: 1920: 1919:Active nuclei 1916: 1908: 1905: 1904: 1903: 1900: 1898: 1895: 1893: 1890: 1888: 1885: 1883: 1880: 1878: 1875: 1873: 1870: 1866: 1863: 1862: 1861: 1858: 1854: 1851: 1850: 1849: 1846: 1844: 1841: 1837: 1834: 1833: 1832: 1829: 1827: 1824: 1822: 1819: 1817: 1814: 1813: 1811: 1807: 1799: 1796: 1795: 1794: 1791: 1789: 1786: 1782: 1779: 1778: 1777: 1774: 1770: 1767: 1766: 1765: 1762: 1758: 1755: 1753: 1750: 1748: 1745: 1743: 1740: 1739: 1738: 1735: 1731: 1728: 1726: 1723: 1721: 1718: 1716: 1713: 1711: 1708: 1706: 1703: 1701: 1698: 1697: 1696: 1693: 1689: 1686: 1684: 1681: 1680: 1679: 1676: 1674: 1671: 1670: 1668: 1666: 1662: 1658: 1651: 1646: 1644: 1639: 1637: 1632: 1631: 1628: 1621: 1617: 1612: 1608: 1607: 1605: 1602: 1599: 1598: 1594: 1591: 1586: 1585:press release 1582: 1581: 1579: 1575: 1573:2 March 2001. 1572: 1568: 1564: 1560: 1559: 1557: 1553: 1548: 1547: 1545: 1542: 1538: 1537: 1533: 1517: 1513: 1509: 1503: 1500: 1487: 1483: 1479: 1473: 1470: 1465: 1461: 1457: 1453: 1449: 1445: 1441: 1437: 1432: 1427: 1423: 1419: 1412: 1409: 1405: 1401: 1397: 1394: 1389: 1386: 1381: 1377: 1372: 1367: 1363: 1359: 1354: 1349: 1345: 1341: 1337: 1330: 1327: 1323: 1319: 1314: 1311: 1306: 1302: 1298: 1294: 1290: 1286: 1282: 1278: 1273: 1268: 1264: 1260: 1253: 1250: 1245: 1241: 1236: 1231: 1227: 1223: 1218: 1213: 1209: 1205: 1201: 1194: 1191: 1186: 1182: 1178: 1174: 1170: 1166: 1161: 1156: 1153:(1): 83–102. 1152: 1148: 1141: 1138: 1125: 1121: 1117: 1111: 1108: 1103: 1099: 1094: 1089: 1085: 1081: 1076: 1071: 1067: 1063: 1059: 1051: 1048: 1043: 1039: 1034: 1029: 1025: 1021: 1017: 1013: 1009: 1005: 1000: 995: 991: 987: 983: 975: 972: 969: 964: 961: 956: 952: 948: 944: 940: 936: 931: 926: 922: 918: 911: 908: 903: 897: 893: 889: 882: 879: 874: 868: 864: 863:W. H. Freeman 860: 853: 850: 845: 841: 837: 833: 829: 825: 821: 817: 810: 808: 804: 793: 789: 783: 780: 773: 769: 766: 764: 761: 759: 756: 754: 751: 749: 746: 744: 741: 739: 736: 735: 731: 725: 722: 719: 716: 712: 710: 707: 706: 703: 700: 697: 694: 690: 688: 685: 684: 681: 677: 674: 671: 668: 664: 662: 659: 658: 655: 652: 649: 646: 642: 640: 637: 636: 633: 630: 627: 624: 620: 618: 615: 614: 611: 608: 605: 602: 598: 596: 593: 592: 589: 586: 583: 580: 576: 574: 571: 570: 567: 564: 561: 558: 554: 552: 549: 548: 545: 542: 539: 536: 532: 530: 527: 526: 523: 520: 517: 514: 510: 508: 505: 504: 501: 498: 495: 492: 488: 486: 483: 482: 479: 478:Constellation 476: 474: 471: 468: 465: 464: 458: 451: 447: 444: 440: 437: 435: 432: 431: 428: 427: 421: 418: 414: 411: 409: 406: 405: 402: 399: 395: 392: 390: 387: 386: 383: 380: 376: 373: 371: 368: 367: 364: 361: 357: 354: 352: 349: 348: 345: 342: 338: 335: 333: 330: 329: 326: 323: 319: 316: 314: 311: 310: 307: 304: 300: 297: 295: 292: 291: 288: 285: 281: 278: 276: 273: 272: 269: 265: 262: 258: 255: 253: 250: 249: 245: 242: 240: 237: 234: 233: 227: 225: 223: 214: 210: 206: 199: 193: 187: 183: 179: 175: 173: 167: 165: 161: 157: 153: 149: 146:, channeling 145: 140: 137: 129: 125: 120: 115: 107: 105: 101: 99: 95: 91: 87: 82: 78: 74: 72: 68: 65:as well. The 64: 60: 56: 52: 51:spiral galaxy 48: 40: 36: 32: 19: 2493:Solar System 2428: 2416: 2151:fossil group 2073:Low activity 1907:Ultramassive 1820: 1737:Dwarf galaxy 1720:intermediate 1715:grand design 1704: 1595: 1520:. Retrieved 1511: 1502: 1490:. Retrieved 1481: 1472: 1421: 1417: 1411: 1388: 1343: 1339: 1329: 1324:, April 2002 1313: 1262: 1258: 1252: 1207: 1203: 1193: 1150: 1146: 1140: 1128:. Retrieved 1119: 1110: 1065: 1061: 1050: 989: 985: 974: 963: 920: 916: 910: 887: 881: 858: 852: 819: 815: 795:. Retrieved 792:ScienceDaily 791: 782: 606:SB(rs)bcpec 423: 246:Information 218: 180: 176: 168: 141: 136:density wave 133: 102: 77:Edwin Hubble 75: 71:Solar System 69:, where the 46: 44: 2481:Outer space 2469:Spaceflight 2210:void galaxy 2173:cannibalism 2158:Interacting 2114:Interaction 2100:Blue Nugget 2090:Dark galaxy 1995:Lyman-break 1887:Protogalaxy 1853:Disc galaxy 1600:April 2002. 1130:12 December 822:: 427–430. 654:Canis Major 370:Messier 108 128:Joseph Lunt 63:spiral arms 2503:Categories 2250:Polar-ring 2095:Red nugget 2037:faint blue 1897:Spiral arm 1752:spheroidal 1742:elliptical 1725:Magellanic 1710:flocculent 1678:Lenticular 1665:Morphology 1522:2017-09-22 1492:6 February 1353:2306.07424 1346:(2): 119. 1272:1906.03916 1075:2210.08658 1068:(1): L10. 999:2311.04283 797:2018-09-17 774:References 724:Horologium 566:Ursa Major 313:Messier 95 156:star birth 154:, fueling 2185:Satellite 2180:Jellyfish 2168:collision 2105:Dead disk 2022:Starburst 1937:Markarian 1809:Structure 1776:Irregular 1747:irregular 1571:SPACE.com 1544:SPACE.com 1456:0004-637X 1431:0710.4552 1380:0004-637X 1305:182953157 1297:0004-6361 1102:2041-8205 1024:1476-4687 844:189840251 687:UGC 12158 213:Andromeda 2417:Category 2306:See also 2230:Galaxies 1957:X-shaped 1788:Peculiar 1730:unbarred 1688:unbarred 1657:Galaxies 1516:Archived 1486:Archived 1464:14841360 1396:Archived 1244:10845683 1185:17562844 1124:Archived 1042:37938777 1033:10651483 955:42162871 732:See also 720:SB(r)ab 709:NGC 1512 639:NGC 2217 617:NGC 1365 595:NGC 7541 588:Eridanus 573:NGC 1300 408:NGC 5398 389:NGC 2903 351:NGC 1073 332:NGC 3953 294:NGC 4921 275:NGC 4314 252:NGC 2787 235:Example 228:Examples 209:NGC 7640 35:NGC 1300 2443:Portals 2277:Quasars 2245:Nearest 2240:Largest 2141:cluster 1974:Seyfert 1436:Bibcode 1358:Bibcode 1277:Bibcode 1265:: A52. 1222:Bibcode 1165:Bibcode 1080:Bibcode 1004:Bibcode 935:Bibcode 923:: 129. 824:Bibcode 753:IC 3447 748:IC 1011 702:Pegasus 124:IC 5201 2429:Portal 2260:Spiral 2163:merger 1942:Quasar 1927:Blazar 1865:corona 1781:barred 1757:spiral 1705:barred 1700:anemic 1695:Spiral 1683:barred 1462:  1454:  1378:  1303:  1295:  1242:  1183:  1100:  1040:  1030:  1022:  986:Nature 953:  898:  869:  842:  680:Tucana 676:Dorado 632:Fornax 610:Pisces 469:Image 434:NGC 55 243:Image 200:Grades 2457:Stars 2297:Voids 2222:Lists 2200:Walls 2136:group 2121:Field 2015:ELIRG 2010:HLIRG 2005:ULIRG 1962:DRAGN 1952:Radio 1932:LINER 1826:Bulge 1798:Polar 1460:S2CID 1426:arXiv 1348:arXiv 1301:S2CID 1267:arXiv 1240:S2CID 1212:arXiv 1181:S2CID 1155:arXiv 1070:arXiv 994:arXiv 951:S2CID 925:arXiv 840:S2CID 584:SBbc 500:Virgo 466:Name 452:(Sm) 412:SBdm 374:SBcd 336:SBbc 298:SBab 194:data. 55:stars 49:is a 41:image 2255:Ring 1860:Halo 1848:Disc 1793:Ring 1673:Disc 1494:2017 1452:ISSN 1376:ISSN 1293:ISSN 1132:2016 1098:ISSN 1038:PMID 1020:ISSN 896:ISBN 867:ISBN 672:SBm 650:SBa 628:SBc 562:SBb 551:M109 540:SBb 518:SBb 496:SBc 473:Type 438:SBm 393:SBd 355:SBc 317:SBb 279:SBa 256:SB0 239:Type 192:WISE 108:Bars 2032:pea 1821:Bar 1444:doi 1422:675 1366:doi 1344:958 1285:doi 1263:629 1230:doi 1208:337 1173:doi 1151:392 1088:doi 1066:945 1028:PMC 1012:doi 990:623 943:doi 921:100 832:doi 820:269 698:SB 544:Leo 529:M95 507:M91 485:M58 424:of 148:gas 2505:: 1769:cD 1583:A 1514:. 1510:. 1484:. 1480:. 1458:. 1450:. 1442:. 1434:. 1420:. 1402:, 1374:. 1364:. 1356:. 1342:. 1338:. 1320:, 1299:. 1291:. 1283:. 1275:. 1261:. 1238:. 1228:. 1220:. 1206:. 1202:. 1179:. 1171:. 1163:. 1149:. 1122:. 1118:. 1096:. 1086:. 1078:. 1064:. 1060:. 1036:. 1026:. 1018:. 1010:. 1002:. 988:. 984:. 949:. 941:. 933:. 919:. 894:. 890:. 865:. 861:. 838:. 830:. 818:. 806:^ 790:. 678:, 224:. 166:. 45:A 2445:: 1649:e 1642:t 1635:v 1613:. 1525:. 1496:. 1466:. 1446:: 1438:: 1428:: 1382:. 1368:: 1360:: 1350:: 1307:. 1287:: 1279:: 1269:: 1246:. 1232:: 1224:: 1214:: 1187:. 1175:: 1167:: 1157:: 1134:. 1104:. 1090:: 1082:: 1072:: 1044:. 1014:: 1006:: 996:: 957:. 945:: 937:: 927:: 904:. 875:. 846:. 834:: 826:: 800:. 130:. 20:)

Index

Barred Spiral galaxy

NGC 1300
Hubble Space Telescope
spiral galaxy
stars
interstellar gas
spiral arms
Milky Way Galaxy
Solar System
Edwin Hubble
Hubble sequence
lenticular galaxy
irregular barred spirals
Magellanic Clouds
elliptical galaxy
Density wave theory § Galactic spiral arms

IC 5201
Joseph Lunt
density wave
stellar nursery
gas
orbital resonance
star birth
active galactic nuclei
Southern Pinwheel Galaxy
supermassive black hole

WISE

Text is available under the Creative Commons Attribution-ShareAlike License. Additional terms may apply.

↑