Photometry of yellow semiregular variables - HR 8752 (= V509 Cassiopeiae)

Details Photometry of yellow semiregular variables - HR 8752 (= V509 Cassiopeiae) Photometry of yellow semiregular variables - HR 8752 (= V509 Cassiopeiae)

Sep 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26a...263..123p&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 263, no. 1-2, p. 123-128.

Astronomy and Astrophysics

Astrophysics

10

Semiregular Variable Stars, Stellar Spectrophotometry, Supergiant Stars, H Ii Regions, Light Curve, Power Spectra, Stellar Color, Stellar Evolution, Stellar Oscillations

Scientific paper

New photoelectric photometry of the yellow semiregular variable HR 8752 (= V509 Cas) made between 1986 and 1991 is presented. Its light curve is very complex, showing a steady decrease in brightness and colors. Period analysis revealed two (possibly three) periods with changing amplitudes. The origin of the amplitude changes may be a change from fundamental to overtone pulsation, though other explanations are equally possible. The evolutionary state of the variable is uncertain. A possible connnection between HR 8752 and the H II zone S151 is pointed out.

Affiliated with

Also associated with

No associations

Rating

Photometry of yellow semiregular variables - HR 8752 (= V509 Cassiopeiae) 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 Photometry of yellow semiregular variables - HR 8752 (= V509 Cassiopeiae), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Photometry of yellow semiregular variables - HR 8752 (= V509 Cassiopeiae) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1761602