Results 1 to 10 of about 82,748 (221)
High Energy Emission of Symbiotic Recurrent Novae: RS Oph and V407 Cyg
Open Astronomy, 2012 Recurrent novae occurring in symbiotic binaries are candidate sources of high energy photons, reaching GeV energies. Such emission is a consequence of particle acceleration leading to pion production.
Hernanz M., Tatischeff V.
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A Demarcation Criterion for Hydrogen Burning of Millinovae
The Astrophysical JournalMillinovae are a new class of transient supersoft X-ray sources with no clear signature of mass ejection. They show similar triangle shapes of V / I band light curves with 1000 times fainter peaks than typical classical novae. Maccarone et al.
Izumi Hachisu, Mariko Kato
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The Vertical Structure of Accretion Disks for Dwarf Novae [PDF]
Journal of Astronomy and Space Sciences, 1985 We have constructed models of steady state accretion disk with accretion rate M=10^16 g/sec or 10^18 g/sec. The mass and the radius of white dwarf were taken as 1 Msolar and 10^9 cm, respectively. The possible application of the results to Z Cha and ZCam
Kyu Hong Choi, Kyung Mee Kim
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Series of Dwarf Nova Outbursts in the Post-novae AT Cancri and GK Persei
The Astronomical JournalAT Cancri and GK Persei are post-novae (Nova Cnc in the seventeenth century and Nova Per 1901). Nowadays, they show episodic brightenings attributed to dwarf nova (DN) outbursts.
Vojtěch Šimon
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A Phenomenon Resembling Early Superhumps in a New SU UMa-type Dwarf Nova with a 2 hr Orbital Period
The Astronomical JournalWe investigate K2BS5, an optical transient that we identified in Campaign 13 of the Kepler/K2 archives by the K2 Background Survey, and classify it as a new SU UMa-type dwarf nova.
Rebecca S. Boyle +6 more
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Mapping edaphic soils' conditions to identify conservation targets for pine barren and sandplain ecosystems in New York State. [PDF]
Ecol Evol, 2022 Corbin JD, Flatland EL.
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Fundamental Properties of Novae in M31
The Astrophysical Journal Supplement SeriesThe peak luminosities and rates of decline for a large sample of novae recently published by Clark et al. have been analyzed using the Yaron et al. nova models to estimate fundamental properties of the M31 nova population.
Allen W. Shafter, Kamil Hornoch
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A Unified Model for Shock Interaction and γ-Ray Emission in Classical Novae
The Astrophysical JournalWe present a parameterized (“toy”) model for shock interaction and γ -ray emission in classical novae, in which a white dwarf envelope of mass M _env is removed over a timescale τ (proportional to the nova speed class, t _2 ) in an outflow that ...
Rebecca Diesing, Brian D. Metzger
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Phosphorus-rich stars with unusual abundances are challenging theoretical predictions. [PDF]
Nat Commun, 2020 Masseron T +6 more
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The Astrophysical JournalA helium nova occurs on a white dwarf (WD) accreting hydrogen-deficient matter from a helium star companion. When the mass of a helium envelope on the WD reaches a critical value, unstable helium burning ignites to trigger a nova outburst.
Mariko Kato, Izumi Hachisu
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