Published March 1988 | Version v1
Journal article Metadata-only

Spectral characteristics of the interstellar molecule H3O+

Creators

Description

The line strengths and probabilities of inversion-rotational transitions of the hydroxonium ion H3O+ are calculated. The expected optical thicknesses of typical interstellar clouds in lines in the radio astronomical range (λ /equal/ 0.8-1.0 mm) are estimated

Additional details

Publishing Information

Journal Title
Astrophysics (English Translation)
Journal Volume
27
Journal Issue
2
Series
Astrophysics (Engl. Transl.).
Journal Page Range
530-535
ISSN
0004-6396
CODEN
ATPYA

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
20070740
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Translation
Descriptors DEI
COSMIC GASES; EINSTEIN COEFFICIENTS; ELECTRIC DIPOLE MOMENTS; ELECTRONIC STRUCTURE; EXCITATION; GROUND STATES; HYDROGEN COMPOUNDS; INFRARED SPECTRA; INTERSTELLAR SPACE; LIFETIME; MOLECULAR IONS; MOLECULAR STRUCTURE; OPTICAL PROPERTIES; OSCILLATOR STRENGTHS; OXYGEN COMPOUNDS; QUANTUM NUMBERS; RADIOWAVE RADIATION; ROTATIONAL STATES; SPIN; VIBRATIONAL STATES
Descriptors DEC
ANGULAR MOMENTUM; CHARGED PARTICLES; DIPOLE MOMENTS; ELECTRIC MOMENTS; ELECTROMAGNETIC RADIATION; ENERGY LEVELS; ENERGY-LEVEL TRANSITIONS; EXCITED STATES; FLUIDS; GASES; IONS; PARTICLE PROPERTIES; PHYSICAL PROPERTIES; RADIATIONS; SPACE; SPECTRA

Optional Information

Notes
Translated from Astrofizika; 27: No. 2, 325-334(Sep-Oct 1987). Cover-to-cover translation of Astrofizika (USSR).