Knowledge (XXG)

Freeman law

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469: 111:, appears in various predicted regularities pertinent to galaxies. For example, it features as an upper cutoff to the mean surface density (or mean surface brightness translated with 510: 411:
Brada, Rafael; Milgrom, Mordehai (December 1998). "The modified dynamics (MOND) predicts an absolute maximum to the acceleration produced by 'dark halos'".
261: 503: 236: 539: 534: 529: 496: 117: 113: 372:"A Mass-Potential Relationship in Elliptical Galaxies and Some Inferences Concerning the Formation and Evolution of Galaxies" 53:. However, after accounting for selection effects, the Freeman law was confirmed in the year 2010 for a sample of 30000 58: 141:
McGaugh, S. S; Bothun, G. D; Schombert, J. M (1995). "Galaxy Selection and the Surface Brightness Distribution".
54: 43: 121:) of galaxies, as observed and formulated in the Freeman law for disks, and of the Fish law for ellipticals. 276:
Fathi, Kambiz (2010). "Revisiting the Scale Length-mu0 Plane and the Freeman Law in the Local Universe".
84:. It was described in 1964 by Robert A. Fish based on photometric results for 29 elliptical galaxies. 430: 383: 342: 295: 207: 160: 476: 446: 420: 311: 285: 176: 150: 39: 80:(or Fish's law) in astronomy is the analogue for the Freeman law with disk galaxies replaced by 240: 255: 81: 480: 438: 391: 350: 303: 215: 168: 93: 434: 387: 346: 299: 211: 164: 307: 50: 468: 523: 450: 315: 180: 35: 355: 330: 62: 17: 425: 155: 331:"The visibility of galaxies as a function of central surface brightness" 49:
More recently it has been argued that the Freeman law is an effect of
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The Freeman law is sometimes called the Fish-Freeman effect.
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The acceleration constant of the modified dynamics (
335:Monthly Notices of the Royal Astronomical Society 98: 42:, ÎŁ at the center. It was described in 1970 by 65:and therefore distance of an observed galaxy. 504: 8: 34:is a statement in astronomy which says that 511: 497: 424: 395: 354: 289: 219: 154: 136: 134: 196:"On the disks of spiral and S0 galaxies" 130: 57:galaxy images. It can be used with the 260:: CS1 maint: archived copy as title ( 253: 7: 465: 463: 483:. You can help Knowledge (XXG) by 329:Disney, M.; Phillipps, S. (1983). 88:Modified Newtonian Dynamics (MOND) 25: 467: 1: 234:Minnesota State University, " 308:10.1088/2041-8205/722/1/L120 194:Freeman, Kenneth C. (1970). 556: 462: 413:The Astrophysical Journal 376:The Astrophysical Journal 278:The Astrophysical Journal 200:The Astrophysical Journal 540:Physical cosmology stubs 370:Fish, Robert A. (1964). 356:10.1093/mnras/205.4.1253 143:The Astronomical Journal 55:Sloan Digital Sky Survey 535:Extragalactic astronomy 530:Observational astronomy 92:According to Brada and 479:-related article is a 123: 27:Astronomical statement 59:Tully–Fisher relation 435:1999ApJ...512L..17B 388:1964ApJ...139..284F 347:1983MNRAS.205.1253D 300:2010ApJ...722L.120F 212:1970ApJ...160..811F 165:1995AJ....110..573M 82:elliptical galaxies 477:physical cosmology 40:surface brightness 492: 491: 61:to determine the 16:(Redirected from 547: 513: 506: 499: 471: 464: 455: 454: 428: 426:astro-ph/9812117 408: 402: 401: 399: 367: 361: 360: 358: 341:(4): 1253–1265. 326: 320: 319: 293: 284:(1): L120–L125. 273: 267: 265: 259: 251: 249: 248: 239:. Archived from 232: 226: 225: 223: 191: 185: 184: 158: 156:astro-ph/9505062 138: 21: 555: 554: 550: 549: 548: 546: 545: 544: 520: 519: 518: 517: 460: 458: 410: 409: 405: 369: 368: 364: 328: 327: 323: 275: 274: 270: 252: 246: 244: 237:"Archived copy" 235: 233: 229: 193: 192: 188: 140: 139: 132: 128: 109: 90: 74: 28: 23: 22: 15: 12: 11: 5: 553: 551: 543: 542: 537: 532: 522: 521: 516: 515: 508: 501: 493: 490: 489: 472: 457: 456: 443:10.1086/311871 403: 397:10.1086/147753 382:(1): 284–305. 362: 321: 268: 227: 221:10.1086/150474 206:(3): 811–830. 186: 173:10.1086/117543 129: 127: 124: 107: 89: 86: 73: 70: 51:selection bias 38:have the same 26: 24: 14: 13: 10: 9: 6: 4: 3: 2: 552: 541: 538: 536: 533: 531: 528: 527: 525: 514: 509: 507: 502: 500: 495: 494: 488: 486: 482: 478: 473: 470: 466: 461: 452: 448: 444: 440: 436: 432: 427: 422: 418: 414: 407: 404: 398: 393: 389: 385: 381: 377: 373: 366: 363: 357: 352: 348: 344: 340: 336: 332: 325: 322: 317: 313: 309: 305: 301: 297: 292: 287: 283: 279: 272: 269: 263: 257: 243:on 2007-07-06 242: 238: 231: 228: 222: 217: 213: 209: 205: 201: 197: 190: 187: 182: 178: 174: 170: 166: 162: 157: 152: 149:(1995): 573. 148: 144: 137: 135: 131: 125: 122: 120: 119: 115: 110: 103: 97: 95: 87: 85: 83: 79: 71: 69: 66: 64: 60: 56: 52: 47: 45: 41: 37: 36:disk galaxies 33: 19: 485:expanding it 474: 459: 416: 412: 406: 379: 375: 365: 338: 334: 324: 281: 277: 271: 245:. Retrieved 241:the original 230: 203: 199: 189: 146: 142: 112: 105: 99: 91: 77: 75: 67: 48: 31: 29: 419:(17): L17. 44:Ken Freeman 32:Freeman law 18:Freeman Law 524:Categories 247:2008-01-11 126:References 63:luminosity 451:117804800 316:119208149 291:1009.2692 181:119527623 256:cite web 78:Fish law 72:Fish law 431:Bibcode 384:Bibcode 343:Bibcode 296:Bibcode 208:Bibcode 161:Bibcode 94:Milgrom 449:  314:  179:  475:This 447:S2CID 421:arXiv 312:S2CID 286:arXiv 177:S2CID 151:arXiv 481:stub 262:link 102:MOND 76:The 30:The 439:doi 417:512 392:doi 380:139 351:doi 339:205 304:doi 282:722 216:doi 204:160 169:doi 147:110 104:), 526:: 445:. 437:. 429:. 415:. 390:. 378:. 374:. 349:. 337:. 333:. 310:. 302:. 294:. 280:. 258:}} 254:{{ 214:. 202:. 198:. 175:. 167:. 159:. 145:. 133:^ 96:, 46:. 512:e 505:t 498:v 487:. 453:. 441:: 433:: 423:: 400:. 394:: 386:: 359:. 353:: 345:: 318:. 306:: 298:: 288:: 266:" 264:) 250:. 224:. 218:: 210:: 183:. 171:: 163:: 153:: 118:L 116:/ 114:M 108:0 106:a 20:)

Index

Freeman Law
disk galaxies
surface brightness
Ken Freeman
selection bias
Sloan Digital Sky Survey
Tully–Fisher relation
luminosity
elliptical galaxies
Milgrom
MOND
M
L


arXiv
astro-ph/9505062
Bibcode
1995AJ....110..573M
doi
10.1086/117543
S2CID
119527623
"On the disks of spiral and S0 galaxies"
Bibcode
1970ApJ...160..811F
doi
10.1086/150474
"Archived copy"
the original

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