Composite spectra. IV - HD 201270/1

Details Composite spectra. IV - HD 201270/1 Composite spectra. IV - HD 201270/1

Sep 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990japa...11..281g&link_type=abstract

Journal of Astrophysics and Astronomy (ISSN 0250-6335), vol. 11, Sept. 1990, p. 281-290. Research supported by SERC, Saint John'

Astronomy and Astrophysics

Astrophysics

6

Binary Stars, Stellar Orbits, Stellar Spectra, Astronomical Spectroscopy, Circular Orbits, Radial Velocity

Scientific paper

HD 201270/1 is a composite-spectrum binary whose components have
spectral types close to G8 III and A2 V. They are in a circular orbit
with a period of only 40 days. Photometric variability of RS CVn
character is therefore not unlikely.

Affiliated with

Also associated with

No associations

Rating

Composite spectra. IV - HD 201270/1 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 Composite spectra. IV - HD 201270/1, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Composite spectra. IV - HD 201270/1 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1404811