Now showing items 1-4 of 4
Particle Asymmetry Analyser
Variability in the UV resonance lines of the cataclysmic variable V795 Herculis (PG-1711 + 336)
Variability in the UV resonance lines from the cataclysmic variable V795 Her is investigated on the basis of a total of 28 IUE SWP low-resolution spectra. Significant line profile fluctuations are evident in the C IV 1549 ...
On the origin of the HI line emission associated with massive young stellar objects
The problem of interpreting the H I line emission associated with massive young stellar objects is addressed by comparing results of LTE calculations of H I Br-alpha and Pf-gamma profiles with observations of the exciting ...