Photometry of chemically peculiar stars (Adelman+ 1998)

Details Photometry of chemically peculiar stars (Adelman+ 1998) Photometry of chemically peculiar stars (Adelman+ 1998)

Sep 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997ycat..41280245a&link_type=abstract

VizieR On-line Data Catalog: J/A+AS/128/245. Originally published in: 1998A&AS..128..245A

Physics

Stars: Peculiar, Photometry: Uvby

Scientific paper

Differential Stroemgren uvby photometric observations from the Four College Automated Photoelectric Telescope are presented for four Chemically Peculiar stars of the upper main sequence: the HgMn star binary AR Aurigae and the magnetic stars 3 Hydrae, 49 Cancri, and BX Bootis. AR Aurigae shows little variability except during the primary and secondary eclipses. The 11.305 day period of Maitzen et al. for 3 Hya is confirmed. A new period of 7.0501 days is found for 49 Cancri while a slightly refined period of 2.88756 days is derived for BX Boo.
(5 data files).

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