A Revision and Update for V1176 Sagitarii

Details A Revision and Update for V1176 Sagitarii A Revision and Update for V1176 Sagitarii

Jun 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991javso..20...68j&link_type=abstract

The Journal of the American Association of Variable Star Observers, vol. 20, no. 1, p. 68-70

Physics

V1176 Sagitarii

Scientific paper

The period of V1176 Sagitarii decreases rapidly, at the rate of 1.36 x
10^-6 days per year. Parabolic elements derived for 1957 to 1990 are:
JD_max = 2441555.368 + 0.35480410 E - 7.0 x 10^-10 E^2. Both the
amplitude and the shape of the light curve change.

Affiliated with

Also associated with

No associations

Rating

A Revision and Update for V1176 Sagitarii 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 Revision and Update for V1176 Sagitarii, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A Revision and Update for V1176 Sagitarii will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1284493