The Magellanic Clouds: Proceedings of the 148th Symposium of the International Astronomical Union, held in Sydney, Australia, July 913, 1990Raymond Haynes, Douglas Milne Springer Science & Business Media, 1991. gada 28. febr. - 503 lappuses Symposium 148 "The Magellanic Clouds and their Dynamical Interaction with the Milky Way" was the first IAU Symposium held in Australia since 1973. In all, 23 countries were represented by 149 participants. The Symposium was held from July 9 to 13, 1990 at Womens College, the University of Sydney. The last symposium on the Magellanic Clouds' was held in 1983 in Ttibingen, Germany. Since then new ground-and satellite-based instruments have become available. A range of results from these instruments were presented at IAU Symposium 148 and are published in these proceedings. IAU Symposium 148 was timed to coincide with the commissioning of the Australia Telescope, and indeed, a few of the first results from that instrument were presented at this Symposium Over the next decade the Australia Telescope is destined to make a major impact on Magellanic Cloud research. Papers are arranged in five main sections reflecting the Symposium timetable: Large-Scale Structure and Kinematics Star Formation and Clustering Stellar Evolution The Interstellar Medium The LMC-SMC-Galaxy System These are preceeded by both the introduction to and the summary of the Symposium. Questions and answers from the oral sessions are reproduced at the end of each section. |
Saturs
V | 17 |
VIII | 20 |
IX | 20 |
X | 20 |
XI | 20 |
XII | 25 |
XIII | 31 |
XIV | 39 |
LXXIX | 285 |
LXXX | 293 |
LXXXI | 301 |
LXXXII | 307 |
LXXXIII | 309 |
LXXXIV | 316 |
LXXXV | 317 |
LXXXVI | 319 |
XV | 45 |
XVI | 47 |
XVII | 51 |
XVIII | 57 |
XIX | 63 |
XX | 65 |
XXI | 71 |
XXII | 75 |
XXIII | 83 |
XXIV | 91 |
XXV | 93 |
XXVI | 95 |
XXVII | 97 |
XXVIII | 99 |
XXIX | 101 |
XXX | 103 |
XXXI | 106 |
XXXII | 108 |
XXXIII | 110 |
XXXIV | 112 |
XXXV | 117 |
XXXVI | 119 |
XXXVII | 132 |
XXXVIII | 133 |
XXXIX | 139 |
XL | 149 |
XLI | 151 |
XLII | 155 |
XLIII | 159 |
XLIV | 165 |
XLV | 171 |
XLVI | 177 |
XLVII | 185 |
XLVIII | 187 |
XLIX | 189 |
L | 190 |
LI | 192 |
LII | 194 |
LIII | 196 |
LIV | 199 |
LV | 201 |
LVI | 203 |
LVII | 205 |
LVIII | 207 |
LIX | 209 |
LX | 211 |
LXI | 213 |
LXII | 216 |
LXIII | 218 |
LXIV | 220 |
LXV | 222 |
LXVI | 224 |
LXVII | 226 |
LXVIII | 228 |
LXIX | 230 |
LXX | 235 |
LXXI | 237 |
LXXII | 243 |
LXXIII | 253 |
LXXIV | 260 |
LXXV | 261 |
LXXVI | 267 |
LXXVII | 273 |
LXXVIII | 279 |
LXXXVII | 321 |
LXXXVIII | 323 |
LXXXIX | 325 |
XC | 328 |
XCI | 331 |
XCII | 333 |
XCIII | 335 |
XCIV | 337 |
XCV | 339 |
XCVI | 341 |
XCVII | 343 |
XCVIII | 345 |
XCIX | 347 |
C | 349 |
CI | 351 |
CII | 354 |
CIII | 357 |
CIV | 359 |
CV | 361 |
CVI | 364 |
CVII | 366 |
CVIII | 368 |
CIX | 370 |
CX | 372 |
CXI | 375 |
CXII | 376 |
CXIII | 378 |
CXIV | 380 |
CXV | 382 |
CXVI | 384 |
CXVII | 385 |
CXVIII | 387 |
CXIX | 390 |
CXX | 393 |
CXXI | 395 |
CXXII | 401 |
CXXIII | 409 |
CXXIV | 415 |
CXXV | 423 |
CXXVI | 425 |
CXXVII | 426 |
CXXVIII | 430 |
CXXIX | 432 |
CXXX | 434 |
CXXXI | 435 |
CXXXIII | 441 |
CXXXIV | 443 |
CXXXV | 447 |
CXXXVI | 457 |
CXXXVII | 463 |
CXXXVIII | 465 |
CXXXIX | 467 |
CXL | 469 |
472 | |
CXLII | 474 |
CXLIII | 477 |
CXLIV | 479 |
CXLV | 481 |
CXLVI | 483 |
CXLVII | 485 |
CXLVIII | 487 |
491 | |
CL | 495 |
Citi izdevumi - Skatīt visu
The Magellanic Clouds: Proceedings of the 148th Symposium of the ... Raymond Haynes,Douglas Milne Priekšskatījums nav pieejams - 1991 |
The Magellanic Clouds: Proceedings of the 148th Symposium of the ... Raymond Haynes,Douglas Milne Priekšskatījums nav pieejams - 1991 |
Bieži izmantoti vārdi un frāzes
30 Doradus abundances Ap.J Astr Astron Astrophys Australia Telescope Bergh carbon stars centre Cepheids Chiosi colours components density derived detected diagram disk distance distance modulus distribution Dopita Dordrecht dredge-up dust emission evolution Feitzinger field Figure flux Galactic Galaxy giant globular clusters halo Haynes HII regions Hodge HVCs IAU Symp infrared interstellar medium ionized Kennicutt kinematics km/s Large Magellanic Cloud LMC and SMC LMC clusters LPVs luminosity Magellanic Cloud LMC Magellanic Stream magnitude main sequence massive stars Mateo Mathewson Meaburn metallicity Milne eds molecular Netherlands observations Observatory obtained OLPVs optical photometry planetary nebulae population radial velocity radio ratio reddening rotation RR Lyraes sample Small Magellanic Cloud spectra star clusters star formation stellar structure supergiants supernova Suppl survey temperature tidal Type variables velocity dispersion Westerlund X-ray