view Abstract Citations References Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Search for Faint OB Stars in the Southern Milky Way. Bok, Bart J. ; Basinski, Jane M. Abstract The new 40-in. reflector for Siding Spring Observatory arrived in Sydney late in January and has been in full operation at the Observatory since early in March. One of its first projects has been the photography of six southern Milky Way fields as a part of a search program for faint early-type stars in the range of apparent magnitude 10 to 15. The search technique is basically that employed earlier at Tonantzintla Observatory. Each photograph on a 103aD emulsion contains three (or more) successive exposures, through a UG2, a GG 13 and a GG 14 filter. Thus are reproduced stellar images on a color system approximating U, B, and V. The 0, B, and A stars are readily located from these plates and their U, B, and V magnitudes and colors are then measured with the aid of single-image 103aO and 103aD plates obtained with the appropriate filters. All of the six are fields for which B. J. Bok and P. F. Bok have now available standard UB V photoelectric sequences to V= 14 or 15, and these sequences permit us to determine precise magnitudes and colors photographically. One of the problems encountered in the rich southern Milky Way fields is that of excessive crowding of the multiple image plates. To supplement the 103aD plates, we have therefore taken on each field a 103aO search plate with two images only, one a 20-min exposure through a UG2 filter, the other a 5-min exposure through a GG 13 filter. Stars with U-B = 0.00 show two images of roughly equal size, stars with U-B <0.00 have a larger U image than a B image. It should be possible to extend the search without much difficulty to V =17, provided good standard photoelectric sequences are available. Publication: The Astronomical Journal Pub Date: 1964 DOI: 10.1086/109385 Bibcode: 1964AJ.....69Q.533B full text sources ADS |