Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
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Page 232
... assumption , with @ , ~ 0 . Which approach is better ? East of the mid - Atlantic ridge , spin equilibrium is a popular choice . Norton and Watson ( 1989b ) gave a thorough discussion of these issues , assumed spin equilibrium , and ...
... assumption , with @ , ~ 0 . Which approach is better ? East of the mid - Atlantic ridge , spin equilibrium is a popular choice . Norton and Watson ( 1989b ) gave a thorough discussion of these issues , assumed spin equilibrium , and ...
Page 233
... assuming that all are in spin equilibrium . The straight line is Eq . ( 21 ) . Error bars show the effect of random errors in Ṁ and M1 . A systematic error from @crit is possible , since μ a writ ( @ crit = 0.6 is assumed ) . 7/6 Most ...
... assuming that all are in spin equilibrium . The straight line is Eq . ( 21 ) . Error bars show the effect of random errors in Ṁ and M1 . A systematic error from @crit is possible , since μ a writ ( @ crit = 0.6 is assumed ) . 7/6 Most ...
Page 346
... assumed distance ( from Wood et al . 1987 , copyright 1987 , American Astronomical Society , reproduced with permission ) . certain that both processes contribute to the increase of nebular mass with time and the assumption that most ...
... assumed distance ( from Wood et al . 1987 , copyright 1987 , American Astronomical Society , reproduced with permission ) . certain that both processes contribute to the increase of nebular mass with time and the assumption that most ...
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abundance additional analysis appear associations assumed Astronomical average binary blue bright calibration catalog central clouds cluster color compared correction derived detection determined discussed distance distribution dwarf eclipse effects emission errors estimate et al evidence evolution field Figure flux frame function galaxies giants given groups included increase indices less light limit lines luminosity magnitude mass mean measured MNRAS nebulae noted objects observations obtained optical orbital PASP period phase photometric pixels position possible present probably quasars range ratio reduced reference region relation relative rotation sample scale scatter secondary shown similar sources spectral spectrum standard stars stellar stellar winds suggests surface survey Table telescope temperature tion University values variability velocity wavelength X-ray