scispace - formally typeset
Open AccessJournal ArticleDOI

Atomic data for astrophysics. I. Radiative recombination rates for H-like, He-like, Li-like, and Na-like ions over a broad range of temperature

Dima Verner, +1 more
- 01 Apr 1996 - 
- Vol. 103, Iss: 2, pp 467-473
Reads0
Chats0
TLDR
In this paper, the authors presented new calculations and analytic fits to the rates of radiative recombination toward H-like, He-like and Li-like ions of all elements from H through Zn.
Abstract
We present new calculations and analytic fits to the rates of radiative recombination toward H-like, He-like, Li-like, and Na-like ions of all elements from H through Zn ({ital Z}=30). The fits are valid over a wide range of temperature, from 3 K to 10{sup 9} K. {copyright} {ital 1996 The American Astronomical Society.}

read more

Content maybe subject to copyright    Report

&61=-9:1;@7.-6;<+3@&61=-9:1;@7.-6;<+3@
&67>4-,/-&67>4-,/-
"0@:1+:)6,:;97675@)+<4;@"<*41+);176: "0@:1+:)6,:;97675@

;751+);).79:;9780@:1+:#),1);1=-#-+75*16);176#);-:;751+);).79:;9780@:1+:#),1);1=-#-+75*16);176#);-:
.79413--413-1413-)6, )413-76:7=-9)97),#)6/-7..79413--413-1413-)6, )413-76:7=-9)97),#)6/-7.
%-58-9);<9-%-58-9);<9-
'-96-9
&61=-9:1;@7.-6;<+3@
)9@-94)6,
&61=-9:1;@7.-6;<+3@
/)9@<3@-,<
7447>;01:)6,),,1;176)4>793:);0;;8:<367>4-,/-<3@-,<80@:):;976(.)+8<*
")9;7.;0-:;9780@:1+:)6,:;97675@75576:)6,;0-"0@:1+:75576:
#1/0;+41+3;778-6).--,*)+3.79516)6->;)*;74-;<:367>07>;01:,7+<5-6;*-6-C;:@7<#1/0;+41+3;778-6).--,*)+3.79516)6->;)*;74-;<:367>07>;01:,7+<5-6;*-6-C;:@7<
#-87:1;79@1;);176#-87:1;79@1;);176
'-96-9)6,-94)6,)9@;751+);).79:;9780@:1+:#),1);1=-#-+75*16);176#);-:.79
413--413-1413-)6, )413-76:7=-9)97),#)6/-7.%-58-9);<9-
"0@:1+:)6,:;97675@
)+<4;@"<*41+);176:

0;;8:<367>4-,/-<3@-,<80@:):;976(.)+8<*
%01:9;1+4-1:*97</0;;7@7<.79.9--)6,78-6)++-::*@;0-"0@:1+:)6,:;97675@);&67>4-,/-;0):*--6
)++-8;-,.7916+4<:17616"0@:1+:)6,:;97675@)+<4;@"<*41+);176:*@)6)<;0791A-,),5161:;9);797.
&67>4-,/-79579-16.795);17684-):-+76;)+;&67>4-,/-4:=<3@-,<

;751+);).79:;9780@:1+:#),1);1=-#-+75*16);176#);-:.79413--;751+);).79:;9780@:1+:#),1);1=-#-+75*16);176#);-:.79413--
413-1413-)6, )413-76:7=-9)97),#)6/-7.%-58-9);<9-413-1413-)6, )413-76:7=-9)97),#)6/-7.%-58-9);<9-
1/1;)4!*2-+;,-6;1C-9!
0;;8,?,7179/
7;-:1;);1766.795);176 7;-:1;);1766.795);176
"<*41:0-,16
%0-:;9780@:1+)47<96)4$<884-5-6;$-91-:
=678
B%0-5-91+)6:;976751+)4$7+1-;@4491/0;:9-:-9=-,
%0-+78@91/0;074,-90):/9)6;-,8-951::176.7987:;16/;0-)9;1+4-0-9-
%01:)9;1+4-1:)=)14)*4-);&67>4-,/-0;;8:<367>4-,/-<3@-,<80@:):;976(.)+8<*

1996ApJS..103..467V

1996ApJS..103..467V

1996ApJS..103..467V

Citations
More filters
Journal ArticleDOI

CLOUDY 90: Numerical Simulation of Plasmas and Their Spectra

TL;DR: In this article, the authors describe version 90 (C90) of the code, paying particular attention to changes in the atomic database and numerical methods that have affected predictions since the last publicly available version, C84.
Journal ArticleDOI

In the Beginning: The First Sources of Light and the Reionization of the Universe

TL;DR: The formation of the first stars and quasars marks the transformation of the universe from its smooth initial state to its clumpy current state as discussed by the authors, and the study of high-redshift sources is likely to attract major attention in observational and theoretical cosmology over the next decade.
Book

Physics of the Interstellar and Intergalactic Medium

TL;DR: In this paper, a comprehensive and richly illustrated textbook on the astrophysics of the interstellar and intergalactic medium is presented, including the gas and dust, as well as the electromagnetic radiation, cosmic rays, and magnetic and gravitational fields, present between the stars in a galaxy and also between galaxies themselves.
Journal ArticleDOI

A comprehensive range of X-ray ionized-reflection models

TL;DR: In this paper, the authors present the results from a comprehensive grid of models computed with their code, which has now been extended to include what they consider to be all energetically important ionization states and transitions.
Journal ArticleDOI

In the Beginning: The First Sources of Light and the Reionization of the Universe

TL;DR: The formation of the first stars and quasars marks the transformation of the universe from its smooth initial state to its clumpy current state as discussed by the authors, and the study of high-redshift sources is likely to attract major attention in observational and theoretical cosmology over the next decade.
Related Papers (5)