The variability of the WC9 Wolf-Rayet star HD 164270

Details The variability of the WC9 Wolf-Rayet star HD 164270 The variability of the WC9 Wolf-Rayet star HD 164270

Jul 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26a...162..109v&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 162, no. 1-2, July 1986, p. 109-113.

Astronomy and Astrophysics

Astrophysics

8

Stellar Spectrophotometry, Variable Stars, Wolf-Rayet Stars, Brightness, Light Curve, Stellar Color, Stellar Luminosity

Scientific paper

The authors present and discuss VBLUW and uvby photometry of the variable WC9 star HD 164270 made in 1981 - 1983. The light variation with an amplitude of ≡0m.1 does not show the double wave with P = 1d.7556 as Isserstedt and Moffat (1981) found in their observations. The large intrinsic scatter superimposed on the double wave is probably one of the reasons for which it is not obvious in the authors' data. A period analysis reveals no other candidate periods. Small colour variations are detected in the VBLUW photometry up to ≡0m.02.

Affiliated with

Also associated with

No associations

Rating

The variability of the WC9 Wolf-Rayet star HD 164270 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 The variability of the WC9 Wolf-Rayet star HD 164270, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The variability of the WC9 Wolf-Rayet star HD 164270 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1654435