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A Composite Light Curve Model of the Symbiotic Nova PU Vul (1979)
DOI: 10.1515/astro-2017-0370 Bibcode: 2012BaltA..21..157K

Mikołajewska, J.; Kato, M.; Hachisu, I.

PU Vul (1979) is a symbiotic nova that shows a long-lasting flat optical peak followed by a slow decline. We made a quasi-evolution model for outbursts on a 0.6 M white dwarf consisting of a series of static solutions with optically-thin winds. Our theoretical models reproduce well the observed visual/UV light curves as well as the new…

2012 Baltic Astronomy
IUE 2
Multiwavelength SED as a Tool in Understanding Outbursts of Symbiotic Binaries
DOI: 10.1515/astro-2017-0363 Bibcode: 2012BaltA..21...97S

Skopal, A.

Symbiotic binaries consist of a few sources of radiation contributing to spectral energy distribution (SED) from hard X-rays to radio wavelengths. To identify the basic physical processes forming the observed spectrum, we have to disentangle the composite SED into its individual components of radiation, i.e., to determine their physical parameters…

2012 Baltic Astronomy
XMM-Newton IUE 0