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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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