uvby phot. of suspected beta Pic-like stars (Nitschelm+, 2000)

Details uvby phot. of suspected beta Pic-like stars (Nitschelm+, 2000) uvby phot. of suspected beta Pic-like stars (Nitschelm+, 2000)

Nov 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000ycat..41450275n&link_type=abstract

VizieR On-line Data Catalog: J/A+AS/145/275. Originally published in: 2000A&AS..145..275N

Other

Stars: Variable, Photometry: Uvby

Scientific paper

We carried out a Stroemgren photometric survey of thirteen southern bright stars, including β Pictoris itself, during three years, d'Astrophysique de Paris, in order to detect possible weak photometric variations. β Pictoris presents a small long-term variation with a change of brightness by -2.1x10-3mag per year, over about two years from beginning of 1996, a situation relatively similar to the one about 18 years ago. Among the other stars, only HD 38392 presents weak photometric variations with a period of 21.4 days, probably related to the star rotation period. The negative result concerning photometric variations of all other stars suggests that those stars are actually really stable and strengthens the reality of the variations discovered in the case of β Pictoris and HD 38392. (2 data files).

Affiliated with

Also associated with

No associations

Rating

uvby phot. of suspected beta Pic-like stars (Nitschelm+, 2000) 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 uvby phot. of suspected beta Pic-like stars (Nitschelm+, 2000), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and uvby phot. of suspected beta Pic-like stars (Nitschelm+, 2000) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1116953