The 53-PERSEI Stars HR:3562 and HR:3600

Details The 53-PERSEI Stars HR:3562 and HR:3600 The 53-PERSEI Stars HR:3562 and HR:3600

Oct 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994mnras.270..914b&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Vol. 270, NO. 4/OCT15, P. 914, 1994

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Scientific paper

The sharp-lined star HR 3562 (B3 IV) has been described as both multiperiodic and singly periodic. It is very likely a member of the 53 Per class (or slowly pulsating B stars). We present intensive photometric observations covering six seasons. The data can be represented by three components with periods 1.957, 2.107 and 2.456 d. HR 3600 (B5 V) is another sharp-lined star which has been described as multiperiodic and a member of the 53 Per class. Our data show that only one period (0.905 d) is present but the true period might be twice this value. Key words: stars: early-type - stars: individual: HR 3562 - stars: individual: HR 3600 - stars: oscillations.

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