1998A&A...331..627L


Query : 1998A&A...331..627L

1998A&A...331..627L - Astronomy and Astrophysics, volume 331627-632 (1998/3-2)

A spectroscopic study of some suspected chemically peculiar stars.

LEONE F. and CATANZARO G.

Abstract (from CDS):

Time-resolved spectra in the 410-700nm range have been obtained to investigate 10 stars which are classified as suspected chemically peculiar stars in The General Catalogue of Ap and Am stars by Renson et al. (1991A&AS...89..429R) or in the latest literature. Among the studied stars, HD 20629 presents metal abundances which are significantly different from main sequence star values and it should be classified as Silicon star. From the HeI587.6 nm line, we conclude that HD 35575 is a helium weak star. Because of the found radial velocity variability and the derived abundances, the periodic photometric variable HD 38602 could be an ellipsoidal variable.

Abstract Copyright: ∼

Journal keyword(s): stars: chemically peculiar - abundances - individual: HD 20629, HD 35575, HD 38602

Simbad objects: 10

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Number of rows : 10
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 V* XX Ari a2* 03 19 47.7617795736 +19 04 34.503922488   7.36 7.41     A0 43 0
2 * tau08 Eri SB* 03 53 42.7023562560 -24 36 44.021417544   4.496 4.623     B6V 123 0
3 V* TU Pic a2* 05 07 25.9269667128 -44 49 18.059792376   6.806 6.892     B5III 51 0
4 HD 35575 * 05 25 36.4983776664 -01 29 28.656465108   6.256 6.420     B5II/III 99 0
5 HD 36629 Y*O 05 32 57.0824474232 -04 33 59.339585016 7.01 7.67 7.65 7.53 7.53 B2V 201 0
6 HD 36589 V* 05 33 38.8369609800 +20 28 27.190778340   6.151 6.189     B6V 55 0
7 * iot Men El? 05 35 36.1786985736 -78 49 15.128878476   6.011 6.033     B8III 56 0
8 HD 60325 * 07 33 22.1853581952 -14 20 17.902042980 5.46 6.17 6.21     B2II 90 0
9 * chi Car bC* 07 56 46.7200933968 -52 58 56.443666728 2.64 3.267 3.431     B3IV 154 1
10 * tet Hya SB* 09 14 21.8600711562 +02 18 51.551915906   3.82   3.9   B9.5V+DA1.6 224 0

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