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HD 152192


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Lists of photometric AM candidates
The Geneva photometric m parameter (Nicolet and Cramer, 1982) is used inorder to select Am photometric candidates from the Rufener (1981)catalogue. Two lists are given, the first containing field stars and thesecond cluster stars. According to the photometric criteria thediffusion process probably responsible for the Am phenomenon takes placerather quickly as Am candidates are present in young clusters. It isconfirmed that the phenomenon is enhanced by low rotational velocity andhigh metallicity. The age seems to slightly affect the Am phenomenon.

Multicolor photometry of metallic-line stars. III. A photometric catalogue
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1974RMxAA...1..175M&db_key=AST

Catalogue of AM stars with known spectral types
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1973A&AS...10..385H&db_key=AST

Catalogue et bibliographie des étoiles A à spectre particulier - Deuxième supplément
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Catalogue et bibliographie des étoiles A à spectre particulier
Not Available

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Gözlemler ve gökölçümü verileri

Takýmyýldýz:Akrep
Sað Açýklýk:16h53m07.06s
Yükselim:-30°25'46.6"
Görünürdeki Parlaklýk:7.031
Uzaklýk:174.825 parsek
özdevim Sað Açýklýk:-12.4
özdevim Yükselim:-1.7
B-T magnitude:7.246
V-T magnitude:7.049

Kataloglar ve belirtme:
Özgün isimleri   (Edit)
HD 1989HD 152192
TYCHO-2 2000TYC 7359-1004-1
USNO-A2.0USNO-A2 0525-24419059
HIPHIP 82598
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