Period study of IT Persei

Details Period study of IT Persei Period study of IT Persei

Apr 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.166..171s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 166, no. 2, April 1990, p. 171-175.

Astronomy and Astrophysics

Astrophysics

Eclipsing Binary Stars, Orbital Elements, Stellar Motions, Light Curve, Stellar Luminosity

Scientific paper

A new period (P = 1.533731 d) of the eclipsing binary system IT Persei is given which is based on all available times of minima. O-C diagrams of IT Persei based on the period given in PPEN (1980) and based on the new period are given. Long-term period changes are not present in the system, however. Some period fluctuations of the order of 10 to the -5th d are seen around the years 1907, 1921, and 1933.

Affiliated with

Also associated with

No associations

Rating

Period study of IT Persei 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 Period study of IT Persei, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Period study of IT Persei will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1379866