Results 51 to 60 of about 370 (81)

Recent progress in understanding the eruptions of classical novae [PDF]

open access: yes
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]

open access: yes
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

open access: yesThe Astrophysical Journal, 1983
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]

open access: yes
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]

open access: yesProc Natl Acad Sci U S A, 2011
Nordhaus J   +4 more
europepmc   +1 more source

MAGELLANIC CLOUDS. XI. SURVEY OF THE NOVAE. [PDF]

open access: yesProc Natl Acad Sci U S A, 1954
Henize KG, Hoffleit D, Nail VM.
europepmc   +1 more source

Nova-like variables [PDF]

open access: yes
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]

open access: yes
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

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