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The Recurrent Novae and Their Relation with Classical Novae
AIP Conference Proceedings, 2002Recurrent novae (RNe) are a subclass of cataclysmic variables classified based on recorded observations of more than one nova outburst. They form a small, but heterogeneous group of objects, with 10 known members, that undergo classical nova‐like outbursts, with the significant differences being in the amplitude and the frequency of the outbursts.
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Interacting Winds in Classical Nova Outbursts
Astrophysics and Space Science, 1995Classical nova outbursts occur in binary systems containing a white dwarf accretor and a Roche-lobe-filling main-sequence star. The outburst is due to a thermonuclear runaway in the accreted material on the surface of the white dwarf, and results in the ejection of up to 10-4M⊙of material at velocities of several hundred to a few thousand kilometres ...
Lloyd, H. M. +2 more
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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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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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The INES Guide for Classical Novae
AIP Conference Proceedings, 2002IUE ULDA/INES Access Guides have been published by ESA since 1989 with the purpose of facilitating the use of IUE data to scientists interested in a specific class of astronomical objects. We present here the “INES Guide for Classical Novae”, in which we shall collect all the available IUE data for a total of 36 novae in outburst and 20 old novae.
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New Insights into Classical Novae
Annual Review of Astronomy and Astrophysics, 2021Brian Metzger +2 more
exaly
Internal shocks from variable outflows in classical novae
Monthly Notices of the Royal Astronomical Society, 2020Brian Metzger +2 more
exaly