A Photometric Investigation of the Short-Period Eclipsing Binary, Nova DQ Herculis (1934).

MF Walker - Astrophysical Journal, vol. 123, p. 68, 1956 - adsabs.harvard.edu
Nova DQ Her (1934) has been found to be an eclipsing binary having the shortest known
period, 4li39 During 1954, 1530 photoelectric observations of the system in three colors …

Structure of envelopes ejected by Novae

ER Mustel, AA Boyarchuk - Astrophysics and Space Science, 1970 - Springer
The paper contains an analysis of the structure of envelopes ejected during the outbursts of
Novae. The data used for this purpose:(a) Direct photographs of envelopes and the …

Photoelectric Observations of Nova DQ Herculis (1934).

MF Walker - Astrophysical Journal, vol. 127, p. 319, 1958 - adsabs.harvard.edu
Observations of DQ Her obtained in 1955 and 1956 are presented. The mni results of this
investigation are as follows: 1. The shape and depth of the eclipse-curve changed between …

On the carbon composition of the ejecta of DQ Herculis

GJ Ferland, JW Truran - Astrophysical Journal, Part 1, vol. 240 …, 1980 - adsabs.harvard.edu
Existing spectrophotometric data for Nova DQ Herculis 1934, spanning virtually its entire
postoutburst history, reveal a time dependence of the inferred nebular composition. The …

[HTML][HTML] On the distance and luminosity of nova DQ Herculis

GJ Ferland - The Observatory, vol. 100, p. 166-167 (1980), 1980 - adsabs.harvard.edu
On the distance and luminosity of nova DQ Herculis ADS Classic is now deprecated. It will be
completely retired in October 2019. This page will automatically redirect to the new ADS …

XV. Analysis of the physical conditions inside the envelope of DQ Herculis 1934

ER Mustel - Vistas in Astronomy, 1974 - Elsevier
A theory of the nova outburst in the course of development of a binary system embedded in
an interstellar cloud has been proposed by Struve (1955) and by Struve and Huang (1957) …