On the new triple-mode pulsating variable star GSC 4018.1807.

Details On the new triple-mode pulsating variable star GSC 4018.1807. On the new triple-mode pulsating variable star GSC 4018.1807.

Oct 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997a%26a...326l...1a&link_type=abstract

Astronomy and Astrophysics, v.326, p.L1-L4

Astronomy and Astrophysics

Astrophysics

12

Stars: Oscillations, Stars: Individual: Gsc 4018.1807

Scientific paper

Variability of GSC 4018.1807 was discovered. The new variable is a triple-mode pulsating star, similar to AC And. Our frequency analysis, based on 895 photographic observations, shows that GSC 4018.1807 has the fundamental (P_0_=0.66887d), first (P_1_=0.51265d) and second (P_2_=0.41103d) overtone pulsation modes as well as non-linear coupling terms (1/P_1_+1/P_0_ and 1/P_1_-1/P_0_). The new variable's period ratio P_1_/P_0_=0.7664 considerably exceeds those typical for bimodal RR Lyr type stars and the ratio observed for AC And.

Affiliated with

Also associated with

No associations

Rating

On the new triple-mode pulsating variable star GSC 4018.1807. 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 On the new triple-mode pulsating variable star GSC 4018.1807., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On the new triple-mode pulsating variable star GSC 4018.1807. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1767985