The photometric and spectroscopic period of the AP star HD 4778

Details The photometric and spectroscopic period of the AP star HD 4778 The photometric and spectroscopic period of the AP star HD 4778

Apr 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26a...159..331h&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 159, no. 1-2, April 1986, p. 331, 332.

Astronomy and Astrophysics

Astrophysics

3

A Stars, Astronomical Photometry, Peculiar Stars, Ubv Spectra, Calcium, Line Spectra, Periodic Variations, Strontium

Scientific paper

The analysis of published photometric and spectroscopic data shows that
the variations are best represented with a period of 2.5481 days,
although a period of 1.64417 days cannot be ruled out.

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