The distance of the Cepheid SU CAS and its pulsation mode

Details The distance of the Cepheid SU CAS and its pulsation mode The distance of the Cepheid SU CAS and its pulsation mode

Aug 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978aj.....83..960s&link_type=abstract

Astronomical Journal, vol. 83, Aug. 1978, p. 960, 961.

Other

11

Cepheid Variables, Nebulae, Stellar Spectrophotometry, Astrometry, Stellar Luminosity, Stellar Mass

Scientific paper

Racine (1968) has used field stars which illuminate reflection nebulae near SU Cas to determine the distance of the Cepheid. These stars have been reobserved in the four-color and H-beta system and found to be at several different distances. If SU Cas is associated with one of them, HD 17706, it must be a first-overtone pulsator. However, since the reflection nebulae in the region appear to be mostly unrelated to each other, the case for overtone pulsation in this star is very weak, and its distance can not be reliably determined in this way.

Affiliated with

Also associated with

No associations

Rating

The distance of the Cepheid SU CAS and its pulsation mode 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 distance of the Cepheid SU CAS and its pulsation mode, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The distance of the Cepheid SU CAS and its pulsation mode will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-943040