2004ApJ...611..598C


Query : 2004ApJ...611..598C

2004ApJ...611..598C - Astrophys. J., 611, 598-604 (2004/August-2)

Experimental and theoretical evaluation of density-sensitive N VI, Ar XIV, and Fe XXII line ratios.

CHEN H., BEIERSDORFER P., HEETER L.A., LIEDAHL D.A., NARANJO-RIVERA K.L., TRABERT E., GU M.F. and LEPSON J.K.

Abstract (from CDS):

The line ratios of the 2p-3d transitions in the boron-like spectra Ar XIV and Fe XXII have been measured using the electron beam ion traps at Lawrence Livermore National Laboratory. Radiative-collisional model calculations show these line ratios to be sensitive to the electron density in the ranges ne=1010-1012/cm3 and ne=1013-1015/cm3, respectively. In our experiment, the electron beam density of about 1011/cm3 was varied by about a factor of 5. Our data show a density effect for the line doublet in Ar XIV, and good agreement with theory is found. The relative intensity of the Fe XXII doublet shows good agreement with our predicted low-density limit. The N VI K-shell spectrum was used to infer the actual electron density in the overlap region of ion cloud and electron beam, and systematic measurements and calculations of this spectrum are presented as well. The Ar XIV and Fe XXII spectra promise to be reliable density diagnostics for stellar coronae, complementing the K-shell diagnostics of helium-like ions.

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Journal keyword(s): Atomic Data - Methods: Laboratory - Sun: Corona - Techniques: Spectroscopic - X-Rays: General

Simbad objects: 4

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Number of rows : 4
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 HD 22468 RS* 03 36 47.2904292073 +00 35 15.943692002 7.09 6.79 5.90     K2:Vnk 1206 0
2 * alf Aur SB* 05 16 41.35871 +45 59 52.7693 1.33 0.88 0.08 -0.52 -0.96 G3III: 1207 0
3 V* EX Hya CV* 12 52 24.2222471899 -29 14 55.999766523   13.505 13.491 13.549   M5-6V 730 0
4 * sig CrB RS* 16 14 40.85557 +33 51 30.9497           F6V+G0V 508 0

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