Disentangling the composite continuum of symbiotic binaries I. S-type systems

Abstract

We describe a method of disentangling the composite,0.12-5 microns continuum of symbiotic binaries.The observed SED is determined by the IUE/HST archival spectra and flux-points corresponding to the optical UBVRI and infrared JHKLM photometric measurements. The modeled SED is given by superposition of fluxes from the cool giant, hot stellar source and nebula including the effect of the Rayleigh scattering process and considering influence of the iron curtain absorptions.We applied this method to 21 S-type symbiotic stars during quiescence, activity and eclipses.

37 pages in printed format, 27 figures, 4 tables, accepted for publication in Astronomy and Astrophysics

References in corpus (3)

• H-alpha variability of the recurrent nova T Coronae Borealis
• X-ray observations of 4 Draconis: symbiotic binary or cataclysmic triple?
• Synthetic Spectral Analysis of the Hot Component in the S-Type Symbiotic Variable EG Andromeda

Cited by in corpus (74)

• Kepler Planet Occurrence Rates for Mid-Type M Dwarfs as a Function of Spectral Type
• A census of symbiotic stars in the 2MASS, WISE and Gaia surveys
• The 2015 super-active state of recurrent nova T CrB and the long term evolution after the 1946 outburst
• Broad H-alpha wings from the optically thin stellar wind of the hot components in symbiotic binaries
• Accretion onto the Companion of Eta Carinae During the Spectroscopic Event: II. X-Ray Emission Cycle
• Spectroscopic binaries among Hipparcos M giants I. Data, orbits, and intrinsic variations
• Structure of the hot object in the symbiotic prototype Z And during its 2000-03 active phase
• On the effect of emission lines on the UBVR photometry
• Rotational velocities of the giants in symbiotic stars: II. Are S-type symbiotics synchronized?
• Transient jets in the symbiotic prototype Z Andromedae
• Recent photometry of symbiotic stars - XII
• Spectroscopic binaries among Hipparcos M giants III. The eccentricity-period diagram and mass-transfer signatures
• The GALAH Survey and Symbiotic Stars. I. Discovery and follow-up of 33 candidate accreting-only systems
• Early evolution of the extraordinary Nova Del 2013 (V339 Del)
• An Online Catalog of Cataclysmic Variable Spectra from the Far Ultraviolet Spectroscopic Explorer
• New outburst of the symbiotic nova AG Peg after 165 years
• The origin of the supersoft X-ray--optical/UV flux anticorrelation in the symbiotic binary AG Draconis
• Wind mass transfer in S-type symbiotic binaries II. Indication of wind focusing
• Recent photometry of symbiotic stars - XIII
• Multiwavelength modelling the SED of supersoft X-ray sources. I. The method and examples
• Wind mass transfer in S-type symbiotic binaries I. Focusing by the wind compression model
• Formation of a disk structure in the symbiotic binary AX Per during its 2007-10 precursor-type activity
• Searching for flickering statistics in T CrB
• Swift observations of the 2015 outburst of AG Peg -- from slow nova to classical symbiotic outburst
• Formation of the Asymmetric Accretion Disk from Stellar Wind Accretion in an S-type Symbiotic Star
• Spectroscopic and photometric analysis of symbiotic candidates -- I. Ten candidates on classical symbiotic stars
• Electron optical depths and temperatures of symbiotic nebulae from Thomson scattering
• Symbiotic stars in X-rays III: Suzaku observations
• Wind mass transfer in S-type symbiotic binaries III. Confirmation of a wind focusing in EG Andromedae from the nebular [OIII]λ5007 line
• Ionization structure of hot components in symbiotic binaries during active phases
• Formation and Evolution of Accreting Compact Objects
• The path to Z And-type outbursts: The case of V426 Sagittae (HBHA 1704-05)
• An X-Ray and Optical Light Curv Model of the Eclipsing Symbiotic Binary SMC3
• Multiwavelength modelling the SED of supersoft X-ray sources. II. RS Ophiuchi: From the explosion to the SSS phase
• Hen 3-860: New southern eclipsing symbiotic star observed in the outburst
• Rms-flux relation and fast optical variability simulations of the nova-like system MV Lyr
• THA 15-31: Discovery with VLT/X-Shooter and Swift/UVOT of a new symbiotic star of the accreting-only variety
• Multiwavelength modeling the SED of nova V339~Del: Stopping the wind and long-lasting super-Eddington luminosity with dust emission
• V618 Sgr: Galactic eclipsing symbiotic nova detected in repeated outbursts
• Repeated transient jets from a warped disk in the symbiotic prototype Z And: A link to the long-lasting active phase
• Broad absorption line symbiotic stars: highly ionized species in the fast outflow from MWC 560
• Period switching in the symbiotic star BX Mon
• The symbiotic star CH Cygni. II. The broad Ly alpha emission line explained by shocks
• Measuring the orbital inclination of Z Andromedae from Rayleigh scattering
• The peculiar light curve of the Symbiotic Star AX Per of the last 125 years
• The GALAH survey: unresolved triple Sun-like stars discovered by the Gaia mission
• Multiwavelength modelling the SED of supersoft X-ray sources III. RS Ophiuchi: The supersoft X-ray phase and beyond
• The symbiotic binary ZZ CMi: intranight variability and suggested outbursting nature
• Stellar Wind Accretion and Raman Scattered O VI Features in the Symbiotic Star AG Draconis
• On the Nature of the Hot Component in the Symbiotic, Supersoft X-ray Binary AG Draconis
• Wind asymmetry imprint in the UV light curves of the symbiotic binary SY Mus
• Symbiotic Stars in the APOGEE Survey: The Case of LIN 358 and SMC N73 (LIN 445a)
• FUSE Spectroscopy of the Accreting Hot Components in Symbiotic Variables
• The symbiotic star CH Cygni. I. An analysis of the shocked nebulae at different epochs
• Formation of a disk-structure and jets in the symbiotic prototype Z And during its 2006-2010 active phase
• Multiwavelength modeling the SED of Luminous Supersoft X-ray Sources in Large Magellanic Cloud and Small Magellanic Cloud
• LIN 358: A symbiotic binary accreting above the steady hydrogen fusion limit
• Notices to investigation of symbiotic binaries V. Physical parameters derived from UBV magnitudes
• PM 1-322: new variable planetary nebula
• Wind-mass transfer in S-type symbiotic binaries IV. Indication of high wind-mass-transfer efficiency from active phases
• Spectrum of the Yellow Symbiotic Star LT Delphini before, during, and after the 2017 Outburst
• The emergence of a neutral wind region in the orbital plane of symbiotic binaries during their outbursts
• Photometry and spectroscopy of the new symbiotic star 2SXPS J173508.4-292958
• Orbital eccentricity of the symbiotic star MWC 560
• Rise and fall of silicate dust in RS Ophiuchi following the 2006 eruption
• Photometry of Symbiotic Stars - XIV
• Density asymmetry and wind velocities in the orbital plane of the symbiotic binary EG Andromedae
• V1047 Cen: The first Z And-type outburst observed in the classical nova binary
• Transient accretion disc-like envelope in the symbiotic binary BF Cygni during its 2006 - 2015 optical outburst
• The applicability of the wind compression model
• Evolved stars as donors in symbiotic binaries
• Second Outburst of the Yellow Symbiotic Star LT Delphini
• AT 2019qyl in NGC 300: Internal Collisions in the Early Outflow from a Very Fast Nova in a Symbiotic Binary
• Photometric Modulations on Intermediate Timescales in the Symbiotic Binaries