[HTML][HTML] The decline and fall of classical novae
J MacDonald, MY Fujimoto… - … ), vol. 294, July 1, 1985, p …, 1985 - adsabs.harvard.edu
The decline and fall of classical novae ADS Classic is now deprecated. It will be completely
retired in October 2019. This page will automatically redirect to the new ADS interface at that …
retired in October 2019. This page will automatically redirect to the new ADS interface at that …
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 …
Novae. The data used for this purpose:(a) Direct photographs of envelopes and the …
The Binary System Nova DQ Herculis. II. an Interpretation of the Spectrum during the Eclipse Cycle.
RP Kraft - Astrophysical Journal, vol. 130, p. 110, 1959 - adsabs.harvard.edu
A model for DQ Her is proposed consisting of a hot, rather bright, white dwarf coupled with a
star that overflows its lobe of the inner Lagrangian surface. Material ejected slowly by the …
star that overflows its lobe of the inner Lagrangian surface. Material ejected slowly by the …
[HTML][HTML] The Binary System Nova DQ Herculis. I. The Spectrum and Radial Velocity during the Eclipse Cycle.
JL Greenstein, RP Kraft - Astrophysical Journal, vol. 130, p. 99, 1959 - adsabs.harvard.edu
The Binary System Nova DQ Herculis. I. The Spectrum and Radial Velocity during t ADS Classic
is now deprecated. It will be completely retired in October 2019. This page will automatically …
is now deprecated. It will be completely retired in October 2019. This page will automatically …
Spectral evolution of Nova Centauri 1986 (V842 Cen)
K Sekiguchi, MW Feast, AP Fairall… - Monthly Notices of the …, 1989 - academic.oup.com
Abstract Spectroscopic observations of Nova Centauri 1986 (V842 Cen) in the optical range
are presented. The spectra at maximum show strong Balmer and Fe ii emission lines with a …
are presented. The spectra at maximum show strong Balmer and Fe ii emission lines with a …
White Dwarf rotation and the shapes of nova remnants
RL Fiedler, TW Jones - Astrophysical Journal, Part 1, vol. 239 …, 1980 - adsabs.harvard.edu
The elongated appearance of many nova remnants is explained due to rapid rotation of the
parent white dwarf. The principal influence of this rotation is seen to be the spin angular …
parent white dwarf. The principal influence of this rotation is seen to be the spin angular …
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) …
an interstellar cloud has been proposed by Struve (1955) and by Struve and Huang (1957) …
[HTML][HTML] The Forbidden Line Spectra of Gaseous Nebulae
MJ Seaton - Gas Dynamics of Cosmic Clouds, 1955 - adsabs.harvard.edu
The Forbidden Line Spectra of Gaseous Nebulae ADS Classic is now deprecated. It will be
completely retired in October 2019. This page will automatically redirect to the new ADS …
completely retired in October 2019. This page will automatically redirect to the new ADS …
[引用][C] CONTRIBUTIONS FROM THE MCDONALD OBSERVATORY
RP KRAFT - Contributions from the McDonald Observatory, Fort …, 1936 - The University
[引用][C] CONTRIBUTIONS FROM THE MCDONALD OBSERVATORY
JL GREENSTEIN, RP KRAFT - Contributions from the McDonald …, 1936 - The University