Results 61 to 70 of about 1,204,542 (190)
A Shocking Shift in Paradigm for Classical Novae
, 2019 The discovery of GeV gamma-rays from classical novae has led to a reassessment of these garden-variety explosions, and highlighted their importance for understanding radiative shocks, particle acceleration, and dust formation in more exotic, distant ...
Linford, Justin +12 more
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The 30P(p, γ)31S reaction in classical novae: progress and prospects
AIP Advances, 2014 The unknown thermonuclear rate of the 30P(p, γ)31S reaction at classical-nova temperatures currently prohibits the accurate modeling of nova nucleosynthesis in the A ⩾ 30 region.
C. Wrede
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Shell Observations of Classical Novae
, 2021 We present shell observations of some classical novae from the Turkish National Observatory. We reobserved them to image their faint shells a long time after their outbursts.
SAYGAÇ, AHMET TALAT +1 more
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Detection of a Molecular Hydrogen Envelope around Nova GK Persei
The Astrophysical Journal LettersThe eruption of Nova Persei 1901 (GK Per) occurred 125 yr ago; remarkably, it still holds major surprises. Using data from the Spectro-Photometer for the History of the Universe, Epoch of Reionization, and Ices Explorer (SPHEREx), we find that it has a ...
D. P. K. Banerjee +6 more
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Optical studies of classical novae in outburst [PDF]
International Astronomical Union Colloquium, 1990 AbstractA nova is followed optically from preoutburst to postoutburst appearance. Photospheric and atmospheric observational data are explained qualitatively through the energy budget, apparent in super-Eddington, Eddington, and sub-Eddington states, and the particle fluxes, according to their role in Grotrian’s model.
openaire +1 more source
, 2018 L'association Artes Novae organise une visite de l'exposition « Naissance de la sculpture gothique. Saint-Denis, Paris, Chartres, 1135-1150 » (10 octobre 2018-21 janvier 2019) conduite par Philippe Plagnieux, professeur en histoire de l'art médiéval ...
Artes Novae
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The space density of classical novae in the galactic disk [PDF]
, 1993 A new determination of the space density of classical novae is presented. Comparison of the properties of nova populations in M3 1, the Galaxy and the LMC, permits to set the outburst rate of novae belonging to the disk of the Galaxy to 5±2.5 novae per ...
DELLA VALLE, Massimo, Duerbeck, H. W.
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Classical Novae – Before and After Outburst [PDF]
International Astronomical Union Colloquium, 1988 Classical nova (CN) and dwarf nova (DN) systems have the same binary components (a low-mass main sequence star and a white dwarf) and the same orbital periods. An important question that therefore arises is: are these systems really different ? (and if so, what is the fundamental difference ?) or, are these the same systems, metamorphosing from one ...
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Rencontre avec Aurélia Cohendy autour de l'exposition "Quand la peinture était dans les livres"
, 2018 L’association Artes Novae a le plaisir de vous inviter à une rencontre avec Aurélia Cohendy autour de l’exposition « Quand la peinture était dans les livres » dont elle a assuré le commissariat avec Magali Vène et qui est présentée à la Bibliothèque d ...
Artes Novae
core
The Astrophysical JournalRecurrent nova (RN) T Pyxidis (T Pyx) has a complex history of mass accreting onto and ejection from the white dwarf, with a classical nova eruption around 1866 kick-starting an RN-phase with six RN eruptions from 1890–2011. T Pyx is a primary progenitor
Bradley E. Schaefer
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