... AM (move to cataclysmics), X, XN, XNB (approximately corresponds to XNG, a B star orbiting a compact object), Xlm (low mass), Xhm (high mass), Xmq (microquasars). ...
... В рамках ГА было проведено 6 симпозиумов МАС : IAUS 316 – Formation, Evolution, and Survival of MassiveStar Clusters ; IAUS 317 – The General Assembly of Galaxy Halos: Structure, Origin and Evolution ; IAUS 318 – Asteroids: New Observations, New Models ...
... A very massive young star surrounded by an expanding gas and dust shell with the diameter 2" at 2mu and 6.5" at 12.2mu. ... The lower massstar, a helium white dwarf, transfers mass to the higher massstar surrounded by an accretion disk. ...
... X, XB, XF, XI, XJ, XND, AM (move to cataclysmics), X, X N, XNB (approximately corresponds to XNG, a B star orbiting a compact object), Xlm (low mass), Xhm (high mass), Xmq (microquasars). ...
... 8] Genzel R. // Strong interstellar masers // in: Masers, molecules and mass outows in star forming regions, ed. A. D. Haschik, Westford, MA: Haytack Obs., 1986, p. 233. ...
... A very massive young star surrounded by an expanding gas and dust shell with the diameter 2" at 2mu and 6.5" at 12.2mu. ... The lower massstar, a helium white dwarf, transfers mass to the higher massstar surrounded by an accretion disk. ...
... In recent years, numerous projects aimed, among other tasks, at the mass automatic discovery of variable stars in fairly extended areas (MACHO, OGLE, ASAS, and others) have been under way. ...
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Ссылки http://www.sai.msu.ru/groups/cluster/gcvs/gcvs/vol1/vol1.pdf -- 558.2 Кб -- 25.07.2002 Похожие документы