Results 101 to 110 of about 1,255,451 (193)
Recurrent Novae, Classical Novae, Symbiotic Novae, and Population II Novae
, 2001 Light curve analysis of decay phase of nova outburst are summarized. Nova duration is determined by the strong wind mass-loss which depends only on the white dwarf mass. Fast novae correspond very massive white dwarfs and very slow novae correspond almost lower mass limit of white dwarfs.
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The Astrophysical JournalV1674 Her is one of the fastest and brightest novae, characterized by dense optical photometry in the premaximum phase—a rise from g = 17 to 7 mag, over one-quarter of a day.
Izumi Hachisu, Mariko Kato
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Prospects for detectability of classical novae with INTEGRAL
, 2001 Classical novae are potential gamma-ray emitters, both in lines and in a continuum. Continuum emission (at energies between 20-30 and 511 keV) and line emission at 511 keV are related to positron annihilation and its Comptonization in the expanding shell; 18F is the main responsible of positron production.
Hernanz, M. +3 more
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, 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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Irradiation-driven Formation of Supersoft X-Ray Sources following Classical Novae
The Astrophysical JournalSupersoft X-ray sources (SSSs) are characterized by persistent thermonuclear burning on the surfaces of white dwarfs (WDs). The standard model requires high mass-transfer rates of ∼10 ^−7 M _⊙ yr ^−1 from massive companions, presenting a theoretical ...
Weitao Zhao +3 more
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Upper Bound of Ejecta Mass in a Nova Outburst
The Astrophysical JournalWe present the maximum ejecta mass ${({M}_{{\rm{ej}}})}_{{\rm{\max }}}$ and the maximum ratio of ejecta mass and accreted mass ${({M}_{{\rm{ej}}}/{M}_{{\rm{acc}}})}_{{\rm{\max }}}$ of a nova for various white dwarf (WD) masses ( M _WD = 0.6–1.38 M _ ...
Izumi Hachisu, Mariko Kato
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Getting to know classical novae with Swift
Journal of High Energy Astrophysics, 2015 11 pages.
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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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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
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Novae in the SuperWASP data base
, 2011 We present the results of trawling through the SuperWASP data base for classical and recurrent novae. We report light curves for a nova in eruption, and for classical novae and a recurrent nova in quiescence.
Pollacco, Don +26 more
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