Results 51 to 60 of about 370 (81)
Recent progress in understanding the eruptions of classical novae [PDF]
Dramatic progress has occurred in the last two decades in understanding the physical processes and events leading up to, and transpiring during the eruption of a classical nova.
Shara, Michael M.
core +1 more source
Celescope catalog of ultraviolet stellar observations. Magnetic tape version [PDF]
Observational results obtained by the celescope experiment during the first 16 months of operation of NASA's Orbiting Astronomical Observatory are presented.
Davis, R. J. +2 more
core +1 more source
H2215-086 -King of the DQ Herculis stars
J. Patterson, J. E. Steiner
openaire +1 more source
Celescope catalog of ultraviolet stellar observations: 5068 objects measured by Orbiting Astronomical Observatory (OAO-2) [PDF]
During the 16 months that the Celescope Experiment operated, it took 8000 frames of data. This report describes the experiment, the data it gathered, the format of the magnetic tape containing the data, and a number of programs that were written to read ...
Davis, R. J. +2 more
core +1 more source
Formation of high-field magnetic white dwarfs from common envelopes. [PDF]
Nordhaus J +4 more
europepmc +1 more source
MAGELLANIC CLOUDS. XII. OBSERVATIONS OF A NOVA IN THE SMALL CLOUD. [PDF]
Smith HJ.
europepmc +1 more source
MAGELLANIC CLOUDS. XI. SURVEY OF THE NOVAE. [PDF]
Henize KG, Hoffleit D, Nail VM.
europepmc +1 more source
Notes on Binary Stars: IV. A Source of Spurious Eccentricity in Spectroscopic Binaries. [PDF]
Sterne TE.
europepmc +1 more source
On grounds of different observable characteristics five classes of nova-like objects are distinguished: the UX Ursae Majoris stars, the antidwarf novae, the DQ Herculis stars, the AM Herculis stars, and the AM Canum Venaticorum stars.
Ladous, Constanze
core +1 more source
Continuum and line spectra of degenerate dwarf X-ray sources [PDF]
Recent observations of X-ray sources are summarized. Unresolved issues concerning these sources are discussed and an outline of the kinds of X-ray observations that would best advance the understanding of these sources is ...
Lamb, D. Q.
core +1 more source

