Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
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Page 187
... values of 8 and A , assumed for photon - noise - limited sensors . The parameter A , is defined by Eqs . ( 31 ) and ( 35 ) . The A , values labeled on this figure are for D = 8 m and sense = 0.6 μm . For other D and Asense values , the ...
... values of 8 and A , assumed for photon - noise - limited sensors . The parameter A , is defined by Eqs . ( 31 ) and ( 35 ) . The A , values labeled on this figure are for D = 8 m and sense = 0.6 μm . For other D and Asense values , the ...
Page 400
... values , and standard deviations are given for the values in several of the columns . 106 : 404-412 , 1994 April CCD Photometry of the. Star V B - V U - B E , Avg 0.54 Min 0.47 Max 0.60 Stdev 0.04 N 12 It is clear that the interstellar ...
... values , and standard deviations are given for the values in several of the columns . 106 : 404-412 , 1994 April CCD Photometry of the. Star V B - V U - B E , Avg 0.54 Min 0.47 Max 0.60 Stdev 0.04 N 12 It is clear that the interstellar ...
Page 479
... values of stars of similar period may be different . Nevertheless , the P√p = Q relation should be valid in the mean in view of the P - L relation exhibited by the variable stars . We assume that this is indeed the case and write the P ...
... values of stars of similar period may be different . Nevertheless , the P√p = Q relation should be valid in the mean in view of the P - L relation exhibited by the variable stars . We assume that this is indeed the case and write the P ...
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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