Fig 3 - uploaded by Werner W. Weiss
Content may be subject to copyright.
The same as Fig. 2 for 1147 "normal" type stars. 

The same as Fig. 2 for 1147 "normal" type stars. 

Source publication
Article
Full-text available
We present Hβ photometry of 233 southern CP2 stars (covering the magnetic Ap stars according to the definition by Preston 1974) brighter than V < 8.5 mag from the list of Bidelman & MacConnell (1973). Absolute magnitudes derived from this photometry together with already existing uvby photometry is confronted with Hipparcos results available for a...

Similar publications

Article
Full-text available
Here we have obtained the {\it BVRI CCD} photometry down to a limiting magnitude of $V \sim$ 20 for the southern poorly studied open cluster NGC 6631. It is observed from the {\it 1.88 m} Telescope of Kottamia Observatory in Egypt. About 3300 stars have been observed in an area of $\sim 10^{\prime} \times 10^{\prime}$ around the cluster center. The...
Article
Full-text available
We present a long-term photometric study of the active K subgiant star CF Oct from 1964 to 1976. It is based on over 350 scanned photographic plates from the Bamberg Observatory plate archive. We performed aperture photometry for the target star and 9 field stars for each plate and did a transformation to standard B magnitude for CF Oct using catal...
Article
Full-text available
The use of the Four College Automatic Photometric Telescope at the Fairborn Observatory in Southern Arizona with its ability to observe stars every clear night and for continuous runs has played a major role in our very successful cooperative program of Strömgren differential uvby photometry of magnetic CP (mCP) stars. Out of about 100 stars observ...
Article
Full-text available
We present the result of a follow-up Strömgren photometric survey of sixteen southern bright stars with circumstellar material, in order to detect possible weak photometric variations. We found new variations of the beta~ Pictoris brightness from 1999 to 2002 with a weak long-term variation of ~-0.8× 10-3 mag per year, over about 3 years. These var...
Article
Full-text available
Albedos for 57 asteroids were determined using diameters obtained from stellar occultations. For 18 objects, the occultation albedos were determined to accuracies better than 5%. The effect on the occultation albedo due to errors in the asteroid absolute magnitude is discussed and correlations between the occultation albedos and IRAS and polarimetr...