A spectroscopic orbit of the late B star 27 Leo

Details A spectroscopic orbit of the late B star 27 Leo A spectroscopic orbit of the late B star 27 Leo

May 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985baicz..36..160h&link_type=abstract

Astronomical Institutes of Czechoslovakia, Bulletin (ISSN 0004-6248), vol. 36, May 1985, p. 160-172.

Astronomy and Astrophysics

Astronomy

B Stars, Orbit Calculation, Orbital Elements, Stellar Orbits, Stellar Spectra, Eccentric Orbits, H Alpha Line, Radial Velocity, Spectrograms, Spectrum Analysis, Stellar Evolution, Visible Spectrum

Scientific paper

The orbital period, 137.3 days and the first orbital elements of the B 9 IV star 27 Leo were derived on the basis of 26 Ondřejov coudé spectrograms, 33 older radial-velocity measurements found in the astronomical literature, and 6 new Victoria spectrograms kindly made available by D. P. Hube. The orbit of the star is highly eccentric and needs further confirmation using more data. Certain suspected spectral peculiarities of the object are briefly discussed. Photometric eclipses of the binary components are not excluded.

Affiliated with

Also associated with

No associations

Rating

A spectroscopic orbit of the late B star 27 Leo 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 A spectroscopic orbit of the late B star 27 Leo, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A spectroscopic orbit of the late B star 27 Leo will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1631586