Photometric period of the AP star HR 3831

Details Photometric period of the AP star HR 3831 Photometric period of the AP star HR 3831

Feb 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26a...131...63r&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 131, no. 1, Feb. 1984, p. 63-66. In French.

Astronomy and Astrophysics

Astrophysics

11

A Stars, Peculiar Stars, Stellar Spectrophotometry, Variable Stars, Binary Stars, Light Curve, Stellar Rotation

Scientific paper

From 32 observations made in February 1977, in the uvby system, a photometric period P = 1.428 + or - 0.005 day was previously found for the A7p SrCrEu star HR 3831 = HD 83368. A series of 26 measurements in December 1975, a few measurements in December 1978, both also in the Stromgren system, and the measurements recently published by Kurtz (1982) in B and V (Johnson system) improve the precision on P. The value obtained is P = 1.42602 + or - 0.00006 day. The photometric variations with this period are displayed. As found previously, a null-wavelength appears in the blue. Kurtz's suggestion that the photometric period is equal to twice the value above does not seem to be justified; however, other considerations favor a rotation period equal to twice the photometric one.

Affiliated with

Also associated with

No associations

Rating

Photometric period of the AP star HR 3831 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 Photometric period of the AP star HR 3831, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Photometric period of the AP star HR 3831 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1857055