Photometric Variability of the Chemically Peculiar Hot Subdwarf LS IV-14 d116

Details Photometric Variability of the Chemically Peculiar Hot Subdwarf LS IV-14 d116 Photometric Variability of the Chemically Peculiar Hot Subdwarf LS IV-14 d116

Jan 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ibvs.5964....1j&link_type=abstract

Information Bulletin on Variable Stars, 5964, 1.

Physics

Scientific paper

We present follow-up photometry of the variable helium-rich and
extremely chemically peculiar subdwarf B star LS IV-14deg 116. These
data confirm the discovery observations, and point to multiple
periodicity with principle periods around 1900 and 3000 s. Further data
are urgently required to secure these results.

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