2008ApJS..179..542P


Query : 2008ApJS..179..542P

2008ApJS..179..542P - Astrophys. J., Suppl. Ser., 179, 542-552 (2008/December-0)

Radiative and auger decay data for modeling Nickel K lines.

PALMERI P., QUINET P., MENDOZA C., BAUTISTA M.A., GARCIA J., WITTHOEFT M.C. and KALLMAN T.R.

Abstract (from CDS):

Radiative and Auger decay data have been calculated for modeling the K lines in ions of the nickel isonuclear sequence, from Ni+ up to Ni27+. Level energies, transition wavelengths, radiative transition probabilities, and radiative and Auger widths have been determined using Cowan's Hartree-Fock with relativistic corrections (HFR) method. Auger widths for the third-row ions (Ni+-Ni10+) have been computed using single-configuration average (SCA) compact formulae.
Result. are compared with data sets computed with the AUTOSTRUCTURE and MCDF atomic structure codes and with available experimental and theoretical values, mainly in highly ionized ions and in the solid state.

Abstract Copyright: ∼

Journal keyword(s): Atomic Data - Atomic Processes - Line: Formation - X-Rays: General

Simbad objects: 11

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Number of rows : 11
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 M 77 Sy2 02 42 40.7091669408 -00 00 47.859690204 9.70 9.61 8.87 10.1 9.9 ~ 4897 2
2 ACO 426 ClG 03 19 47.6 +41 30 54           ~ 2508 1
3 ACO 478 ClG 04 13 24.8 +10 27 52           ~ 522 0
4 Z 329-24 Sy2 06 15 36.2812259376 +71 02 14.837219808 14.21 14.03 12.97     ~ 960 2
5 V* GP Vel HXB 09 02 06.8608812864 -40 33 16.899168060 6.85 7.37 6.87 6.31 6.05 B0.5Ia 1588 0
6 NAME Centaurus A BLL 13 25 27.61521044 -43 01 08.8050291   8.18 6.84 6.66   ~ 4774 3
7 NAME Circinus Galaxy Sy2 14 13 09.906 -65 20 20.47   10.89 9.84 10.6 10.0 ~ 1331 1
8 IGR J16318-4848 HXB 16 31 48.3090342864 -48 49 00.665054832         16.217 B[e]I 181 0
9 NAME Galactic Center reg 17 45 39.60213 -29 00 22.0000           ~ 16269 0
10 V* V5512 Sgr LXB 18 14 31.3 -17 09 23     12.73     K5III 449 0
11 V* V1405 Aql LXB 19 18 47.6 -05 14 18 20.90 21.40 21.0     ~ 495 0

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