On the possible presence of promethium in the spectra of HD 101065 (przybylski's star) and HD 965

Astronomy and Astrophysics

Volumn 419, Issue 3, 2004, Pages 1087-1093

  Cowley, C R ^a   Bidelman, W P ^b   Hubrig, S ^c   Mathys, G ^c   Bord, D J ^d  

^a UNIVERSITY OF MICHIGAN   (United States)

^b CASE WESTERN RESERVE UNIVERSITY   (United States)

^c EUROPEAN SOUTHERN OBSERVATORY   (Chile)

^d UNIVERSITY OF MICHIGAN DEARBORN   (United States)

Author keywords

Methods: data analysis; Stars: abundances; Stars: activity; Stars: atmospheres; Stars: chemically peculiar

Indexed keywords

DATA REDUCTION; GALAXIES; OBSERVATORIES; PROBABILITY; PROMETHIUM; RADIOISOTOPES; SURFACE PHENOMENA;

ATMOSPHERIC METHODS; CHEMICALLY PECULIAR STARS; STARS;

ASTROPHYSICS;

EID: 2542459246     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20035726     Document Type: Article

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