The determination of the orbital elements and masses of stars in the close binary system V 367 Cygni

Details The determination of the orbital elements and masses of stars in the close binary system V 367 Cygni The determination of the orbital elements and masses of stars in the close binary system V 367 Cygni

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989pazh...15..247g&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 15, March 1989, p. 247-252. In Russian. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

Binary Stars, Cygnus Constellation, Orbital Elements, Stellar Mass, Stellar Orbits, Line Spectra, Radial Velocity, Stellar Spectra

Scientific paper

Positional measurements of the only stellar line Mg II 4481 A in the spectrum of V 367 Cyg were carried out using high-dispersion spectrograms. The secondary component of the line, which shows displacement corresponding to the motion of the companion is identified. The radial velocities of both components were measured and the elements of the spectral orbit and mass of the stars were calculated to be M1 = 2.3 solar masses and M2 = 3.6 solar masses.

Affiliated with

Also associated with

No associations

Rating

The determination of the orbital elements and masses of stars in the close binary system V 367 Cygni 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 The determination of the orbital elements and masses of stars in the close binary system V 367 Cygni, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The determination of the orbital elements and masses of stars in the close binary system V 367 Cygni will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1528098