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1992
Nova shells are formed from material which is ejected form the surface of a White Dwarf during an outburst. The shells contain usually about 10−5 solar masses and expand with velocities of some hundreds to more than thousand km/s. They reflect the chemical composition of the White Dwarf, the material accreted from the secondary of the binary system ...
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Nova shells are formed from material which is ejected form the surface of a White Dwarf during an outburst. The shells contain usually about 10−5 solar masses and expand with velocities of some hundreds to more than thousand km/s. They reflect the chemical composition of the White Dwarf, the material accreted from the secondary of the binary system ...
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X-ray nova candidates among old classical novae
Astrophysics, 1999A review of light curves of known x-ray novae made it possible to identify criteria by which x-ray nova candidates were selected among old novae: amplitude of optical outburst 7–10m, shape of light curve during the outburst with a temporary fading by 2–3m lasting up to four days and an abrupt final fading from the 6m level (relative to the quiet state).
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BATSE observations of classical novae
AIP Conference Proceedings, 2000Detection of gamma-ray emission from classical novae, in the range between 30 and 511 keV, would provide a crucial test of the thermonuclear runaway (TNR) model. This emission results from the annihilation of positrons, emitted by some radioactive nuclei (13N and 18F) synthesized during the TNR; it has a short duration and is produced before the ...
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New Insights into Classical Novae
Annual Review of Astronomy and Astrophysics, 2021Laura Chomiuk +2 more
exaly
Synthesis of radioactive elements in novae and supernovae and their use as a diagnostic tool
New Astronomy Reviews, 2021Jordi Isern +2 more
exaly
Nucleosynthesis Accompanying Classical Nova Outbursts
1986Theoretical studies of thermonuclear runaways in degenerate hydrogen-rich matter leading to classical nova outbursts predict that nova ejecta can be characterized by substantial overabundances of the elements carbon, nitrogen, and oxygen as well as of other interesting nuclear species.
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Observations of galactic and extragalactic novae
Astronomy and Astrophysics Review, 2020Massimo Della Valle, Luca Izzo
exaly
Population synthesis of accreting white dwarfs: rates and evolutionary pathways of H and He novae
Monthly Notices of the Royal Astronomical Society, 2021Alexander Kemp +2 more
exaly