Zobrazeno 1 - 10
of 12
pro vyhledávání: '"M. S. Barbour"'
Autor:
W. C. Priedhorsky, M. S. Barbour, I. G. Nolt, James C. Kemp, E. N. Walker, D. J. Kraus, G. D. Henson, J. Terrell, J. V. Radostitz
Publikováno v:
The Astrophysical Journal. 271:L65
Autor:
M. S. Barbour, James C. Kemp
Publikováno v:
The Astrophysical Journal. 246:203
Using measurements on 79 nights in 1980 January-August, it is established that the polarization in the ultraviolet (U band) varies synchronously on the known binary period of 2.6132 days, with a peak-to-peak amplitude of 0.03%. The pattern is mainly
Publikováno v:
The Astrophysical Journal. 273:L85
Autor:
J. C. Kemp, M. S. Barbour
Publikováno v:
Publications of the Astronomical Society of the Pacific. 93:521
The use of photoelastic polarimeters in astronomy is briefly reviewed, and a visible and near-UV photoelastic modulation polarimeter is described which has been in continuous service on the 61-cm telescope of Pine Mountain Observatory for 6 years. Th
Publikováno v:
The Astrophysical Journal. 275:247
Publikováno v:
The Astrophysical Journal. 220:L123
Using 180 nights of data from 1975 and 1977, we have found a stable polarization variation in the V band which is periodic on the orbital cycle of 5/sup d/.600. The peak-to-peak amplitude is 0.25% and is largely in the position-angle Stokes parameter
Publikováno v:
The Astronomical Journal. 83:962
Publikováno v:
The Astrophysical Journal. 238:L133
Photometry covering 100 nights during 1979 July-November is reported, in an unfiltered band (effectively 5200-8000 A), in a V band, and with a few measures in B. Correlation with the 13 day period of Crampton, Cowley, and Hutchings is found in the fo
Autor:
J. C. Kemp, M. S. Barbour
Publikováno v:
The Astrophysical Journal. 264:237
Observations of periodicities in the optical polarization of the weak X-ray source X Persei are reported. Polarization was measured in the V band 400 times over the course of 356 nights during 1977-1982. The Q and U Stokes parameters derived from the
Publikováno v:
The Astrophysical Journal. 243:557
Results of a study of the phase-locked optical polarization of the Algol triple star system are presented. Polarimetry was obtained in the B filter during 75 nights from 1979 to 1980, and results were folded on the AB orbital period for the equatoria