The Kα complex of He-like iron with dielectronic satellites

被引:32
作者
Oelgoetz, J
Pradhan, AK
机构
[1] Ohio State Univ, Dept Chem, Columbus, OH 43210 USA
[2] Ohio State Univ, Dept Astron, Columbus, OH 43210 USA
关键词
atomic data; atomic processes; line : profiles; galaxies : Seyfert; X-rays : galaxies;
D O I
10.1046/j.1365-8711.2001.04980.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
It is shown that the dielectronic satellites (DES) dominate X-ray spectral formation in the 6.7-keV K alpha complex of Fe XXV at temperatures below that of maximum abundance in collisional ionization equilibrium T-m. Owing to their extreme temperature sensitivity, the DES are excellent spectral diagnostics for T < T-m in photoionized, collisional or hybrid plasmas; whereas the forbidden, intercombination and resonance lines of Fe XXV are not. A diagnostic line ratio GD(T) is defined including the DES and the lines, with parameters from new relativistic atomic calculations. The DES absorption resonance strengths may be obtained from differential oscillator strengths, possibly to yield the Fe XXIV/Fe XXV column densities. The DES contribution to highly ionized Fe should be of interest for models of redward broadening of K<alpha> features, ionized accretion discs, accretion flows and Ka temporal-temperature variability in AGN.
引用
收藏
页码:L42 / L46
页数:5
相关论文
共 42 条
[31]   RECOMBINATION-CASCADE X-RAY-SPECTRA OF HIGHLY CHARGED HELIUM-LIKE IONS [J].
PRADHAN, AK .
ASTROPHYSICAL JOURNAL, 1985, 288 (02) :824-830
[32]   DENSITY AND TEMPERATURE DIAGNOSTICS OF X-RAY SOURCES - LINE RATIOS FOR HELIUM-LIKE IONS [J].
PRADHAN, AK ;
SHULL, JM .
ASTROPHYSICAL JOURNAL, 1981, 249 (02) :821-830
[33]   Radiation damping of autoionizing resonances [J].
Pradhan, AK ;
Zhang, HL .
JOURNAL OF PHYSICS B-ATOMIC MOLECULAR AND OPTICAL PHYSICS, 1997, 30 (17) :L571-L579
[34]   ON THE SYSTEMATICS OF LINE RATIOS ALONG THE HELIUM ISOELECTRONIC SEQUENCE [J].
PRADHAN, AK .
ASTROPHYSICAL JOURNAL, 1982, 263 (01) :477-482
[35]   X-ray photoabsorption in KLL resonances of OVI and abundance analysis [J].
Pradhan, AK .
ASTROPHYSICAL JOURNAL, 2000, 545 (02) :L165-L169
[36]   GRAVITATIONALLY REDSHIFTED EMISSION IMPLYING AN ACCRETION DISK AND MASSIVE BLACK-HOLE IN THE ACTIVE GALAXY MCG-6-30-15 [J].
TANAKA, Y ;
NANDRA, K ;
FABIAN, AC ;
INOUE, H ;
OTANI, C ;
DOTANI, T ;
HAYASHIDA, K ;
IWASAWA, K ;
KII, T ;
KUNIEDA, H ;
MAKINO, F ;
MATSUOKA, M .
NATURE, 1995, 375 (6533) :659-661
[37]  
Vainshtein L. A., 1978, Atomic Data and Nuclear Data Tables, V21, P49, DOI 10.1016/0092-640X(78)90003-7
[38]   HIGH-RESOLUTION X-RAY SPECTROSCOPIC EVIDENCE OF NONEQUILIBRIUM CONDITIONS IN THE CYGNUS LOOP [J].
VEDDER, PW ;
CANIZARES, CR ;
MARKERT, TH ;
PRADHAN, AK .
ASTROPHYSICAL JOURNAL, 1986, 307 (01) :269-274
[39]   X-RAY-LINE EMISSION FROM THE PUPPIS A SUPER-NOVA REMNANT - OXYGEN LINES [J].
WINKLER, PF ;
CANIZARES, CR ;
CLARK, GW ;
MARKERT, TH ;
PETRE, R .
ASTROPHYSICAL JOURNAL, 1981, 245 (02) :574-580
[40]   Physical diagnostics from a narrow FeKα emission line detected by Chandra in the Seyfert 1 galaxy NGC 5548 [J].
Yaqoob, T ;
George, IM ;
Nandra, K ;
Turner, TJ ;
Serlemitsos, PJ ;
Mushotzky, RF .
ASTROPHYSICAL JOURNAL, 2001, 546 (02) :759-768