Received: 2011-11-23
Accepted: 2011-11-25
Published Online: 2017-3-23
Published in Print: 2012-6-1
© 2017
Articles in the same Issue
- The Asiago Astrophysical Observatory and the Recently Refurbished 1.22 m Galileo telescope
- Symbiotic Stars: Observations Confront Theory
- The ANS Collaboration Monitoring Program
- Characterizing the Photometric Response of the ANS Collaboration Monitoring Program
- The Search for Symbiotic Stars in the IPHAS Survey
- New Symbiotic Stars Monitored with the Hermes Spectrograph: A Case Study of Orbital Hα Modulation
- Spectroscopic Observations of the Recurrent Symbiotic Nova V407 Cyg During 2001 - 2009
- The X-Ray Evolution of the Symbiotic Star V407 Cyg During its 2010 Outburst
- High Energy Emission of Symbiotic Recurrent Novae: RS Oph and V407 Cyg
- An Extremely Massive White Dwarf of the Symbiotic Classical Nova V407 Cyg as Suggested by the RS Oph and U SCO Models
- Hydrodynamic Studies of the Evolution of Recurrent, Symbiotic and Dwarf Novae: the White Dwarf Components are Growing in Mass
- Mass Transfer in Mira-Type Binaries
- Multiwavelength SED as a Tool in Understanding Outbursts of Symbiotic Binaries
- Formation of Neutral Disk-Like Zone Around the Active Hot Stars in Symbiotic Binaries
- Mass Ejection from the Symbiotic Prototype Z and During its 2006 Outburst
- RR Tel: Determination of Dust Properties During Minimum Obscuration
- News from AG Draconis
- The Long-Term Spectroscopic Misadventures of AG Dra with a Nod Toward V407 Cyg: Degenerates Behaving Badly
- Symbiotic Nova PU Vul - 33 Years of Observations
- A Composite Light Curve Model of the Symbiotic Nova PU Vul (1979)
- Mass Transfer in Two Post-AGB Binaries with Dusty Disks
- Spectroscopic Monotoring of the Symbiotic Star BX Monocerotis
- Reconstructing Historical Light Curves of Symbiotic Stars and Novae
- Abell-35 Phenomena in Symbiotic Stars: Discovery of 1.2 and 6.4 Day Periods in VV8 (V471 Per)
- Photometric Activity of the Symbiotic Star CH Cyg During 2008–2011
- BF Cyg During its Current Outburst
- Telescope and Researcher Potential of Turkey for Collaboration in CV Studies
- Contribution of the Electron Scattering Process to the Broad Hα Wings
- SBS 0802+529: A New Variable Star from the Second Byurakan Survey
- On the Symbiotic X-Ray Binary Nature of the Star CGCS 5926
Keywords for this article
stars;
binaries;
symbiotic;
fundamental parameters;
mass-loss
Creative Commons
BY-NC-ND 4.0
Articles in the same Issue
- The Asiago Astrophysical Observatory and the Recently Refurbished 1.22 m Galileo telescope
- Symbiotic Stars: Observations Confront Theory
- The ANS Collaboration Monitoring Program
- Characterizing the Photometric Response of the ANS Collaboration Monitoring Program
- The Search for Symbiotic Stars in the IPHAS Survey
- New Symbiotic Stars Monitored with the Hermes Spectrograph: A Case Study of Orbital Hα Modulation
- Spectroscopic Observations of the Recurrent Symbiotic Nova V407 Cyg During 2001 - 2009
- The X-Ray Evolution of the Symbiotic Star V407 Cyg During its 2010 Outburst
- High Energy Emission of Symbiotic Recurrent Novae: RS Oph and V407 Cyg
- An Extremely Massive White Dwarf of the Symbiotic Classical Nova V407 Cyg as Suggested by the RS Oph and U SCO Models
- Hydrodynamic Studies of the Evolution of Recurrent, Symbiotic and Dwarf Novae: the White Dwarf Components are Growing in Mass
- Mass Transfer in Mira-Type Binaries
- Multiwavelength SED as a Tool in Understanding Outbursts of Symbiotic Binaries
- Formation of Neutral Disk-Like Zone Around the Active Hot Stars in Symbiotic Binaries
- Mass Ejection from the Symbiotic Prototype Z and During its 2006 Outburst
- RR Tel: Determination of Dust Properties During Minimum Obscuration
- News from AG Draconis
- The Long-Term Spectroscopic Misadventures of AG Dra with a Nod Toward V407 Cyg: Degenerates Behaving Badly
- Symbiotic Nova PU Vul - 33 Years of Observations
- A Composite Light Curve Model of the Symbiotic Nova PU Vul (1979)
- Mass Transfer in Two Post-AGB Binaries with Dusty Disks
- Spectroscopic Monotoring of the Symbiotic Star BX Monocerotis
- Reconstructing Historical Light Curves of Symbiotic Stars and Novae
- Abell-35 Phenomena in Symbiotic Stars: Discovery of 1.2 and 6.4 Day Periods in VV8 (V471 Per)
- Photometric Activity of the Symbiotic Star CH Cyg During 2008–2011
- BF Cyg During its Current Outburst
- Telescope and Researcher Potential of Turkey for Collaboration in CV Studies
- Contribution of the Electron Scattering Process to the Broad Hα Wings
- SBS 0802+529: A New Variable Star from the Second Byurakan Survey
- On the Symbiotic X-Ray Binary Nature of the Star CGCS 5926