Published December 1, 1990 | Version v1
Journal article

Hydrogen stark profiles for astrophysics

Creators

  • 1. Department Atomes et Moleules en Astrophysique et URA812 du CNRS Observatoires de Paris, 5 Place. J. Janssen, 92195 Meudon Cedex, France (France)

Description

A large number of hydrogen line profiles are calculated in the framework of the model microfield method with specific modification for electronic contributions. Profiles of the Lyman, Balmer and Paschen series have been obtained from the center to the Holtsmark wings of the lines

Additional details

Publishing Information

Journal Title
AIP Conference Proceedings
Journal Volume
216
Journal Issue
1
Series
AIP Conf. Proc.
Journal Page Range
607-608
ISSN
0094-243X
CODEN
APCPC

Conference

Title
10. international conference on spectral line shapes.
Dates
25-29 Jun 1990.
Place
Austin, TX (USA).

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
22052754
Subject category
S74: ATOMIC AND MOLECULAR PHYSICS; S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Conference
Descriptors DEI
HYDROGEN; HYDROGEN IONS; LYMAN LINES; PLASMA DENSITY; SPECTRAL SHIFT; STARK EFFECT; STELLAR ATMOSPHERES
Descriptors DEC
ATMOSPHERES; CHARGED PARTICLES; ELEMENTS; IONS; NONMETALS

Optional Information

Secondary number(s)
CONF-9006278--.