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    <subfield code="a">SCART-2021-0065</subfield>
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    <subfield code="a">Trust, O.</subfield>
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    <subfield code="a">Starspots and rotation velocities of normal A- and Am- stars</subfield>
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    <subfield code="c">2020</subfield>
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    <subfield code="a">Neiner C., Weiss W.W., Baade D., Griffin R.E., Lovekin C.C., Moffat A.F.J. (eds.) </subfield>
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    <subfield code="a">Using the ``hump and spike'' features, we computed the rotation frequencies and amplitudes. The corresponding equatorial rotational velocity (Vrot) and spot size were estimated. On fitting the autocorrelation functions of the light-curves with the appropriate model, we obtained the starspot decay-time scale. The Vrot agrees well with the projected rotational velocity (νsin i) in the literature. Considering a single circular and black spot, we estimate its radius from the amplitude of the ``spike''. No evidence for a significant difference in the average ``spike'' amplitude and spot radius was found for Am/Fm and normal A stars. Indeed, we derived an average value of ∼21±2 and ∼19±2 ppm for the photometric amplitude and of 1.01±0.13 and 1.16±0.12 R_E for the spot radius (where R_E is the Earth radius), respectively. We do find a significant difference for the average spot decay-time scale, which amounts to 3.6±0.2 and 1.5±0.2 days for Am/Fm and normal A stars, respectively. In general, spots on normal A stars are similar in size to those on Am/Fm stars, and both are weaker than previously estimated. The existence of the ``spikes'' in the frequency spectra may not be strongly dependent on the appearance of starspots on the stellar surface. In comparison with G, K and M stars, spots in normal A and Am/Fm stars are weak which may indicate the presence of a weak magnetic field. </subfield>
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    <subfield code="a">NO</subfield>
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  <datafield tag="653" ind1="1" ind2=" ">
    <subfield code="a">Stars: photometry</subfield>
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  <datafield tag="653" ind1="1" ind2=" ">
    <subfield code="a">Stars: chemically peculiar</subfield>
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  <datafield tag="653" ind1="1" ind2=" ">
    <subfield code="a">Stars: rotation</subfield>
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  <datafield tag="653" ind1="1" ind2=" ">
    <subfield code="a">Stars: starspots</subfield>
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  <datafield tag="700" ind1=" " ind2=" ">
    <subfield code="a">Jurua, E.</subfield>
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  <datafield tag="700" ind1=" " ind2=" ">
    <subfield code="a">De Cat, P.</subfield>
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    <subfield code="a">Joshi, S.</subfield>
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  <datafield tag="773" ind1=" " ind2=" ">
    <subfield code="p">Proceedings of the International Conference on Stars and their Variability Observed from Space, pp. 353-354 (2020)</subfield>
    <subfield code="y">2020</subfield>
    <subfield code="c">433-434</subfield>
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    <subfield code="f">peter.decat@observatoire.be</subfield>
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    <subfield code="a">https://ui.adsabs.harvard.edu/abs/2020svos.conf..433T/abstract</subfield>
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    <subfield code="s">202531</subfield>
    <subfield code="u">http://publi2-as.oma.be/record/5285/files/Trust2020_SVOSconf_433.pdf</subfield>
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    <subfield code="a">published in</subfield>
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    <subfield code="a">NONREF</subfield>
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