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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absorption abundance accretion analysis asteroids astrometry Astronomical Society binary bright calibration catalog central star chromospheric clouds color comets correction derived detection detector diagram disk distribution eclipse emission errors estimate evolution expansion velocities Fe/H field flux frame function galactic galaxies GCLF giant branch globular clusters H II regions Hyades indices infrared ionized km s¹ light curve lines luminosity magnitude main sequence main-sequence mass measured MNRAS objects observations Observatory obtained open clusters optical orbital parameters PASP period phase photometric pixels planetary nebulae plotted quasars radial velocities radius range ratio red giants reddening redshift region residuals rotation sample scale scatter secondary solar sources spectral type spectroscopic spectrum standard stellar subgiant survey Table telescope temperature tion turnoff values variability wavelength white dwarf width X-ray XX Vir