Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
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Page 365
... secondary is -1.7 ± 0.3 dex . The secondary is not significantly underabundant in N or O. We interpret the C deficiency of the secondary as a result of mass transfer , which has removed its outer layers and exposed its CN - processed ...
... secondary is -1.7 ± 0.3 dex . The secondary is not significantly underabundant in N or O. We interpret the C deficiency of the secondary as a result of mass transfer , which has removed its outer layers and exposed its CN - processed ...
Page 366
... secondary of V356 Sgr and a standard star ( HR 7145 ) . The observation of V356 Sgr was made when the A2 II secondary totally eclipsed the B3 V primary . The C1 lines are evident in the spectrum of HR 7145 , but , with the exception of ...
... secondary of V356 Sgr and a standard star ( HR 7145 ) . The observation of V356 Sgr was made when the A2 II secondary totally eclipsed the B3 V primary . The C1 lines are evident in the spectrum of HR 7145 , but , with the exception of ...
Page 373
... secondary of V356 Sgr and a standard star ( HR 7145 ) . The observation of V356 Sgr was made when the A2 II secondary totally eclipsed the B3 V primary . The C1 lines are evident in the spectrum of HR 7145 , but , with the exception of ...
... secondary of V356 Sgr and a standard star ( HR 7145 ) . The observation of V356 Sgr was made when the A2 II secondary totally eclipsed the B3 V primary . The C1 lines are evident in the spectrum of HR 7145 , but , with the exception of ...
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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