Results 111 to 120 of about 125,367 (265)

A 70 pc Diameter Nova Superremnant Surrounding the Recurrent Nova RS Ophiuchi

open access: yesThe Astronomical Journal
Recurrent novae undergo thermonuclear-powered eruptions separated by less than 100 yr, enabled by subgiant or red giant donors transferring hydrogen-rich matter at very high rates onto their massive white dwarf companions.
Michael M. Shara   +11 more
doaj   +1 more source

Spectroscopic Identification and Population Properties of Cataclysmic Variables from DESI DR1

open access: yesThe Astrophysical Journal Supplement Series
We present a systematic search for cataclysmic variables (CVs) using spectroscopic data from Data Release 1 of the Dark Energy Spectroscopic Instrument. Applying the Bagging-TopPush algorithm, we identified 433 CV candidates and related objects, of which
Wen Hou   +5 more
doaj   +1 more source

High Energy Emission of Symbiotic Recurrent Novae: RS Oph and V407 Cyg

open access: yesOpen 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.
doaj   +1 more source

Search for 22Na in novae supported by a novel method for measuring femtosecond nuclear lifetimes. [PDF]

open access: yesNat Commun, 2023
Fougères C   +61 more
europepmc   +1 more source

A Photoionization Model for the Infrared Coronal Line Emission in the Classical Nova V1716 Scorpii

open access: yesThe Astrophysical Journal
A near-infrared spectrum of nova V1716 Scorpii (PNV J17224490-4137160), a recent bright ( ${V}_{\max }=7.3$ mag), Fermi-LAT detected γ -ray source, was modeled using the photoionization code CLOUDY.
C. E. Woodward   +4 more
doaj   +1 more source

The Vertical Structure of Accretion Disks for Dwarf Novae [PDF]

open access: yesJournal 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
doaj  

MULTI-TIME-SCALE VARIABILITY OF STARS

open access: yesOdessa Astronomical Publications, 2017
Physical mechanisms and corresponding mathematical models for different types of stellar variability are reviewed with applications to concrete stars.
I. L. Andronov
doaj   +1 more source

A radio-detected type Ia supernova with helium-rich circumstellar material. [PDF]

open access: yesNature, 2023
Kool EC   +36 more
europepmc   +1 more source

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