Results 111 to 120 of about 86,009 (222)
The recurrent novae and their relation with classical novae
, 2002 Recurrent novae (RNe) are a subclass of cataclysmic variables classified based on recorded observations of more than one nova outburst. They form a small, but heterogeneous group of objects, with 10 known members, that undergo classical nova‐like ...
Anupama, G. C.
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A radio-detected type Ia supernova with helium-rich circumstellar material. [PDF]
Nature, 2023 Kool EC +36 more
europepmc +1 more source
Datasets for the article "Transient behavior of three SU UMa-type dwarf novae; AR Pic, QW Ser and V521 Peg"
Szegedi, Helene +3 more
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The Astronomical JournalWe present photometric and spectroscopic studies of a new WZ Sagittae (Sge)-type dwarf nova (DN) KSP-OT-202104a discovered by the Korea Microlensing Telescope Network Supernova Program. The source exhibits outburst amplitudes of ∼8 mag with a duration of
Sang Chul Kim +6 more
doaj +1 more source
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
doaj
Hubble space telescope STIS spectroscopy of long-period dwarf novae in quiescence
, 2008 We present the results of a synthetic spectral analysis of HST STIS spectra of five long-period dwarf novae obtained during their quiescence to determine the properties of their white dwarfs, which are little known for systems above the CV period gap ...
deMartino, Domitilla +9 more
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Application of the hot white dwarf atmosphere models to the X-ray data of classical novae
, 2021 The analyses of X-ray emission from classical novae after outburst have shown that the soft X-ray emission below 1 keV, which is thought to originate from the photosphere of the white dwarf, is inconsistent with the simple black body model of emission ...
BALMAN, Şölen
core
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
doaj +1 more source
88th Annual Meeting of the Meteoritical Society 2026: Abstracts
Meteoritics &Planetary Science, Volume 61, Issue S1, Page S48-S551, August 2026.
wiley +1 more source