Photometric variability of the binary HD 1826

Details Photometric variability of the binary HD 1826 Photometric variability of the binary HD 1826

May 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987rmxaa..14..410g&link_type=abstract

(IAU, Reunion Regional Latinoamericana de Astronomia, 5th, Merida, Mexico, Oct. 6-10, 1986) Revista Mexicana de Astronomia y Ast

Astronomy and Astrophysics

Astronomy

Astronomical Photometry, Binary Stars, Light Curve, Stellar Luminosity, Variable Stars, Fourier Analysis, Radial Velocity

Scientific paper

Photoelectric two-color measurements of the single-lined spectroscopic binary HD 1826 are presented showing its photometric variability. The period of the light variations has been found to be in excellent agreement with the orbital period derived from the radial velocity measurements. An estimation of the amplitude of the variations of 0.03 mag has been obtained roughly independent of color. The system appears to be an ellipsoidal variable and the available preliminary results are discussed in light of the most probable binary model.

Affiliated with

Also associated with

No associations

Rating

Photometric variability of the binary HD 1826 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Photometric variability of the binary HD 1826, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Photometric variability of the binary HD 1826 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-860646