Lists of photometric AM candidates

Details Lists of photometric AM candidates Lists of photometric AM candidates

Feb 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983a%26as...51..245n&link_type=abstract

Astronomy and Astrophysics Supplement Series, vol. 51, Feb. 1983, p. 245-256.

Astronomy and Astrophysics

Astrophysics

5

A Stars, Metallic Stars, Peculiar Stars, Stellar Spectrophotometry, Correlation Coefficients, Star Clusters, Stellar Rotation, Tables (Data)

Scientific paper

The Geneva photometric m parameter (Nicolet and Cramer, 1982) is used in order to select Am photometric candidates from the Rufener (1981) catalogue. Two lists are given, the first containing field stars and the second cluster stars. According to the photometric criteria the diffusion process probably responsible for the Am phenomenon takes place rather quickly as Am candidates are present in young clusters. It is confirmed that the phenomenon is enhanced by low rotational velocity and high metallicity. The age seems to slightly affect the Am phenomenon.

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