Photometric Studies of Asteroids. VIII. Additional Photographic Magnitudes.
Abstract
view Abstract Citations (4) References (5) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Photometric Studies of Asteroids. VIII. Additional Photographic Magnitudes. Gehrels, T. ; Carstens, J. R. ; Peters, J. G. ; Peters, L. S. Abstract In the Yerkes-McDonald Asteroid Survey, photographic magnitudes were determined brighter than P0 = 16.5. For fainter asteroids and for some with large inclination and eccentricity additional magnitudes are reported in this paper. The work was done as a part of the regular Indiana Asteroid Program, supplemented by plates taken in South Africa. Aspect variation and its effects on the precision of photometry are discussed. The axes of rotation of the asteroids are apparently fixed in space. Asteroids may be used in order to transfer the zero point of the U, B, V system from the northern to the southern hemispheres. Publication: The Astrophysical Journal Pub Date: July 1960 DOI: 10.1086/146917 Bibcode: 1960ApJ...132..232G full text sources ADS | Related Materials (12) Part 1: 1954ApJ...120..200G Part 2: 1954ApJ...120..529G Part 3: 1954ApJ...120..547S Part 4: 1954ApJ...120..551A Part 5: 1956ApJ...123..331G Part 6: 1957ApJ...125..550G Part 7: 1958ApJ...127..253V Part 8: 1960PGLO...37...53G Part 10: 1960ApJ...132..915G Part 11: 1962ApJ...135..906G Part 12: 1962PGLO...46..906G Part 13: 1963PGLO...53.1279W
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