Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
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Page 288
... velocity approaches 100 km s - 1 . The velocity system for the correlations using the sky template has the same zero point as the correlations using the new calculated templates to within 0.1 km s - 1 . The initial selection of stars ...
... velocity approaches 100 km s - 1 . The velocity system for the correlations using the sky template has the same zero point as the correlations using the new calculated templates to within 0.1 km s - 1 . The initial selection of stars ...
Page 503
... velocity distribution of the smallest 25 % of the 244 nebulae having both radius and velocity known is shown in Fig . 3. This sample consists of 62 nebulae with linear radii of Rion≤0.05 pc . The expansion - velocity distribution of ...
... velocity distribution of the smallest 25 % of the 244 nebulae having both radius and velocity known is shown in Fig . 3. This sample consists of 62 nebulae with linear radii of Rion≤0.05 pc . The expansion - velocity distribution of ...
Page 506
... velocity of the original AGB wind , and where M and exp ( PNN ) are the mass - loss rate and expansion velocity of the fast wind of the PN nucleus . Values of Vexp ( PN ) are given for various values of U exp ( AGB ) and for constant ...
... velocity of the original AGB wind , and where M and exp ( PNN ) are the mass - loss rate and expansion velocity of the fast wind of the PN nucleus . Values of Vexp ( PN ) are given for various values of U exp ( AGB ) and for constant ...
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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