EDP Sciences
Free Access
Volume 419, Number 3, June I 2004
Page(s) 1087 - 1093
Section Stellar atmospheres
DOI https://doi.org/10.1051/0004-6361:20035726
Published online 07 May 2004

A&A 419, 1087-1093 (2004)
DOI: 10.1051/0004-6361:20035726

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

C. R. Cowley1, W. P. Bidelman2, S. Hubrig3, G. Mathys3 and D. J. Bord4

1  Department of Astronomy, University of Michigan, Ann Arbor, MI 48109-1010, USA
2  Department of Astronomy, Case Western Reserve University, Cleveland, OH 44106-7215, USA
3  European Southern Observatory, Casilla 19001, Santiago 19, Chile
    e-mail: [shubrig; gmathys]@eso.org
4  Department of Natural Sciences, University of Michigan-Dearborn, Dearborn, MI 48128-1491, USA
    e-mail: dbord@umd.umich.edu

(Received 21 November 2003 / Accepted 23 February 2004 )

Traditional and statistical line-identification methods indicate the presence of Pm I and II, Tc I, and perhaps Tc II in the spectrum of the roAp star HD 101065. These methods also lead to the presence of Pm II and probably also Pm I in a related cool Ap star, HD 965. The spectroscopic evidence is strong enough that we would declare promethium to be present without hesitation, if any of its isotopes were stable. The longest-lived promethium isotope has a half-life of only 17.7 years. The presence of this element would mean that unrecognized processes - perhaps flare activities - are taking place in the atmospheres of these stars. The significance of such processes for galactic chemical evolution cannot be ruled out. We discuss the possibility that the highly improbable wavelength coincidences are due to chance, or due to contamination of the laboratory sources.

Key words: stars: chemically peculiar -- stars: abundances -- stars: activity -- stars: atmospheres -- methods: data analysis

Offprint request: C. R. Cowley, cowley@umich.edu

SIMBAD Objects

© ESO 2004

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.