2005MNRAS.356.1256C


Query : 2005MNRAS.356.1256C

2005MNRAS.356.1256C - Mon. Not. R. Astron. Soc., 356, 1256-1262 (2005/February-1)

An elemental abundance analysis of the magnetic chemically peculiar star HR 8216.

CALISKAN H.

Abstract (from CDS):

An elemental abundance analysis of the cool magnetic CP star HR 8216 (= HD204411) was performed using 2.4 Å/mm Dominion Astrophysical Observatory Reticon exposures covering λλ3830-4770 with a typical signal-to-noise ratio of 200 taken with the long camera of the 1.22-m telescope. The spectrograms were measured interactively with the graphics computer program reduce. The fine analysis used an ATLAS9 metal-rich model atmosphere, the predictions of which best-matched the optical region fluxes and the Hγ profile. The anomalies of HR 8216 are primarily an enhancement of many iron peak elements with the rare earths elements much less enhanced than in many similar cool magnetic CP stars. Using the results of the fine analysis the spectrum was synthesized. Comparison with the observed spectrum showed that the agreement is good but did not fully account for all of the observed line spectrum.

Abstract Copyright: 2004 RAS

Journal keyword(s): stars: abundances - stars: chemically peculiar - stars: individual: HR 8216

VizieR on-line data: <Available at CDS (J/MNRAS/356/1256): table6.dat>

Simbad objects: 6

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Number of rows : 6
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* HN And a2* 01 24 18.6765786624 +43 08 31.629475248   6.704 6.676     A4VpSrSi 153 0
2 V* PP Vir a2* 14 04 48.9376773456 +05 24 51.459774732   8.70 8.29     F0 86 0
3 * alf Cir a2* 14 42 30.4206520931 -64 58 30.478845491 3.55 3.43 3.19 2.96 2.86 A7VpSrCrEu 384 0
4 V* V694 CrA a2* 18 12 25.8347418984 -37 45 09.271268532   8.34 7.92     ApSrCrEu 122 0
5 * gam Equ a2* 21 10 20.5000721160 +10 07 53.691967776 5.03 4.94 4.68 4.43 4.32 A9VpSrCrEu 564 0
6 HD 204411 a2* 21 26 51.6219389280 +48 50 06.599806584 5.54 5.38 5.31     A4VpSiCrHg 190 0

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