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The Infrared Temporal Development of Classical Novae
Annual Review of Astronomy and Astrophysics, 1988L'examen des donnees IR existantes concernant les novae permet de decrire les processus physiques qui caracterisent leur developpement post-eruptif, d'identifier les parametres qui distinguent les differents scenarii, de discuter les theories sur l'evolution des systemes binaires serres, de decrire les processus de condensation de la poussiere dans les
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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, 2021Laura Chomiuk +2 more
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Internal shocks from variable outflows in classical novae
Monthly Notices of the Royal Astronomical Society, 2020Elad Steinberg, Brian D Metzger
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