Results 81 to 90 of about 86,009 (222)
Low-metallicity Nova Explosions: A Site for Weak rp-process Nucleosynthesis
The Astrophysical JournalClassical novae are common cataclysmic events involving a binary system of a white dwarf and a main-sequence or red giant companion star. In metal-poor environments, these explosions produce ejecta differently from their solar counterparts due to the ...
Athanasios Psaltis +3 more
doaj +1 more source
Crop, Forage &Turfgrass Management, Volume 12, Issue 1, June 2026.Abstract With the growth in the craft brewing industry, farmers are interested in producing winter malting barley (Hordeum vulgare L.). Timely barley planting is important; however, wet weather often results in delays. The objective of this experiment was to identify the agronomic optimum seeding rate (the seeding rate at which yield is maximized) for ...
Laura E. Lindsey +2 more
wiley +1 more source
The Astrophysical JournalFor Galactic novae, I calculate and collect a comprehensive catalog of 208 measures of white dwarf (WD) masses ( M _WD ) and 232 measures of average V magnitudes in quiescence ( V _q ). These are collected into a comprehensive catalog of most fundamental
Bradley E. Schaefer
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DETECTION OF SUPERHUMPS IN THE DWARF NOVA PV PERSEI
Odessa Astronomical Publications, 2017 The CBA (Center for Backyard Astrophysics) Belgium Observatory belongs to a global network of small photometric telescopes, that study periodic phenomena in Cataclysmic Variables (CVs).
T. Vanmunster
doaj +1 more source
Mammal Community Responses to Increasing Puma Activity in a Suburban Preserve
Ecology and Evolution, Volume 16, Issue 6, June 2026.Using nine years of camera‐trap data from a suburban preserve, we found preliminary, convergent evidence that increasing puma activity coincided with changes in black‐tailed deer, bobcat and coyote activity. Evidence for changes in brush rabbit and grey fox activity, as well as woody plant density, is more tentative and warrants further study, but ...
Chinmay Sonawane +7 more
wiley +1 more source
Spectroscopic analysis of the dwarf nova SS Cygni
, 2010 Dwarf novae are a type of cataclysmic variable in which one of the components is a white dwarf. Their outbursts can range in brightness from two to five magnitudes at intervals that can vary from days to decades. The purpose of this study is to analyze
Benson-Avillan, Elixia.
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, 1993 Recurrent novae seem to be a rather inhomogeneous group: T CrB is a binary with a M III companion; U Sco probably has a late dwarf as companion. Three are fast novae; two are slow novae. Some of them appear to have normal chemical composition; others may
Selvelli, Pierluigi, Hack, Margherita
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OUTBURST CYCLICITY OF DWARF NOVA VZ AQUARII
Odessa Astronomical Publications, 2017 New linear elements for outbursts of VZ Aqr from 1904 to 1987 were obtained with P0 = 50.4053d. Two states of outburst activity are distinguished with cycle lengths 47.128d and 55.041d, replacing each other during Π = 13.2yr and accompanied by a maximum ...
L. I. Shakun
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On the occurrence of dwarf nova outbursts in post novae
, 2000 accepted for publication in Astronomy and ...
Schreiber, M. R. +2 more
openaire +3 more sources
, 2018 Fondée en mars 2018, Artes Novae est l'association des jeunes chercheur(e)s en archéologie et histoire de l'art du Moyen Âge et de la Renaissance, actifs en Île-de-France.
Artes Novae
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