Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
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Page 25
... stars cannot yet be observed . In addition to many individual papers , a number of recent conference proceedings ... stars , as they were called then , for the entire galactic plane and remarked on their distribution , as did EdFIG ...
... stars cannot yet be observed . In addition to many individual papers , a number of recent conference proceedings ... stars , as they were called then , for the entire galactic plane and remarked on their distribution , as did EdFIG ...
Page 35
... star is less than 2 million years old . The spread is at least 8 million years . This figure also demonstrates that the presence of low - mass ( 3-5M ) stars on or very close to the main sequence is not a particularly interesting ...
... star is less than 2 million years old . The spread is at least 8 million years . This figure also demonstrates that the presence of low - mass ( 3-5M ) stars on or very close to the main sequence is not a particularly interesting ...
Page 301
... stars in the giant branch of NGC 752. Filled symbols are binaries , squares are stars without Li estimates , triangles are stars with upper limits to Li , and circles are stars with measurable Li . face temperature declines . At a ...
... stars in the giant branch of NGC 752. Filled symbols are binaries , squares are stars without Li estimates , triangles are stars with upper limits to Li , and circles are stars with measurable Li . face temperature declines . At a ...
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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