HD 59435 Geneva photometry (Wade+, 1999)

Details HD 59435 Geneva photometry (Wade+, 1999) HD 59435 Geneva photometry (Wade+, 1999)

Apr 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999ycat..33470164w&link_type=abstract

VizieR On-line Data Catalog: J/A+A/347/164. Originally published in: 1999A&A...347..164W

Computer Science

Stars: Ap, Photometry: Geneva

Scientific paper

The SB2 binary HD 59435 hosts a yellow giant and a magnetic Ap star, the latter being the secondary (Wade et al., 1996, Cat. ) and exhibiting spectral lines resolved into their magnetically-split components. Additional measurements of the magnetic field modulus of the Ap secondary are reported, as well as additional radial velocities for both components and photometric magnitudes and colours in the Geneva system. The magnetic field modulus varies with a period of about 1360 days. For a general description of the Geneva photometric system, see e.g. (1 data file).

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