Results 1 to 10 of about 85,351 (144)
Reconstructing Historical Light Curves of Symbiotic Stars and Novae
Open Astronomy, 2012 We reconstructed photometric histories of symbiotic stars and novae from direct inspection and measurement of photographic plates preserved at historical archives.
Ulisse Munari, Rajka Jurdana-Šepić
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Infrared Spectroscopy of Symbiotic Stars. IX. D-Type Symbiotic Novae [PDF]
Astrophysical Journal, 2013 Time-series spectra of the near-infrared 1.6 {mu}m region have been obtained for five of the six known D-type symbiotic novae. The spectra map the pulsation kinematics of the Mira component in the Mira-white dwarf binary system and provide the center-of-mass velocity for the Mira.
Peter Wood +2 more
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Eruptive Novae in Symbiotic Systems [PDF]
Monthly Notices of the Royal Astronomical Society, 2023 ABSTRACTWe conduct numerical simulations of multiple nova eruptions in detached, widely separated symbiotic systems that include an asymptotic giant branch (AGB) companion to investigate the impact of white dwarf (WD) mass and binary separation on the evolution of the system.
Yael Hillman +2 more
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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.
Margarita Hernanz, V Tatischeff
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The Structure of the Envelopes of Symbiotic Novae [PDF]
Lecture Notes in Physics, 1990 Symbiotic novae are composite spectrum stars whose light history is characterized by one single major outburst. At high resolution their optical and UV spectra are very rich of emission lines belonging to a wide ionization range. Generally one can identify both narrow and broad line systems.
R Viotti
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MULTI-FREQUENCY STUDY OF SYMBIOTIC NOVAE
Odessa Astronomical Publications, 2017 Symbiotic novae are subclass of symbiotic stars - interacting binaries with wide orbits, whose photometric history is characterized by a single nova- like outburst lasting decades and caused by a thermonuclear runaway on the surface of a wind accreting ...
D. Chochol, T. Pribulla
doaj +3 more sources
Open Astronomy, 2012 Symbiotic binaries are systems containing white dwarfs (WDs) and red giants. Symbiotic novae are those systems in which thermonuclear eruptions occur on the WD components.
Francis Timmes +2 more
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Near-Infrared and Ultraviolet Spectrophotometry of Symbiotic Novae [PDF]
Astrophysical Journal, Supplement Series, 1999 ABSTRACTIn this paper we present an atlas of near-infrared spectrophotometry of symbiotic novae and reportresults from nearly contemporaneous IUE observations. The data cover RT Ser, AG Peg, V1016 Cyg,V1329 Cyg, HM Sge, and Pu Vul, most of the known symbiotic novae that are observable from thenorthern hemisphere.
Peter Erwin +2 more
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The outbursts of symbiotic novae [PDF]
The Astrophysical Journal, 1983 We discuss possible conditions under which thermonuclear burning episodes in the hydrogen-rich envelopes of accreting white dwarfs give rise to outbursts similar in nature to those observed in the symbiotic stars AG Peg, RT Ser, RR Tel, AS 239, V1016 Cyg, V1329 Cyg, and HM Sge.
S. J. Kenyon, J. W. Truran
openaire +2 more sources
Theoretical Light-curve Models of the Symbiotic Nova CN Cha—Optical Flat Peak for 3 Yr
The Astrophysical Journal, 2023 CN Cha is a slow symbiotic nova characterized by a 3 yr long optical flat peak followed by a rapid decline. We present theoretical light curves for CN Cha, based on hydrostatic approximation, and estimate the white-dwarf (WD) mass to be ∼0.6 M _☉ for a ...
Mariko Kato, Izumi Hachisu
doaj +1 more source