Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
From inside the book
Results 1-3 of 83
Page 264
... standard stars in the center of M15 , plotted against apparent visual magnitude ( a ) – ( d ) and apparent B - V color ( e ) - ( h ) . Residuals are shown for ( a ) , ( e ) the instrumental u band ; ( b ) , ( f ) the instrumental b band ...
... standard stars in the center of M15 , plotted against apparent visual magnitude ( a ) – ( d ) and apparent B - V color ( e ) - ( h ) . Residuals are shown for ( a ) , ( e ) the instrumental u band ; ( b ) , ( f ) the instrumental b band ...
Page 265
... standard stars in the center of M15 , plotted against apparent visual magnitude ( a ) – ( d ) and apparent B – V color ( e ) – ( h ) . Residuals are shown for ( a ) , ( e ) the instrumental u band ; ( b ) , ( f ) the instrumental b band ...
... standard stars in the center of M15 , plotted against apparent visual magnitude ( a ) – ( d ) and apparent B – V color ( e ) – ( h ) . Residuals are shown for ( a ) , ( e ) the instrumental u band ; ( b ) , ( f ) the instrumental b band ...
Page 510
... standard star data in Table 1 with the Strömgren b - y system ( Hauck and Mermilliod 1980 ) . This has been made possible by the high quality of the standard - star data and the predominance of early - type dwarfs in the standard - star ...
... standard star data in Table 1 with the Strömgren b - y system ( Hauck and Mermilliod 1980 ) . This has been made possible by the high quality of the standard - star data and the predominance of early - type dwarfs in the standard - star ...
Other editions - View all
Common terms and phrases
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