Abstract
A history of the 1.22 m Galileo telescope of the Asiago Astrophysical Observatory is described.
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Open Astronomy
formerly Baltic Astronomy
Editor-in-Chief: Barbuy, Beatriz
IMPACT FACTOR 2018: 0.350
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- The Asiago Astrophysical Observatory and the Recently Refurbished 1.22 m Galileo telescope
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- The ANS Collaboration Monitoring Program
- Characterizing the Photometric Response of the ANS Collaboration Monitoring Program
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- New Symbiotic Stars Monitored with the Hermes Spectrograph: A Case Study of Orbital Hα Modulation
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- 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
The Asiago Astrophysical Observatory and the Recently Refurbished 1.22 m Galileo telescope
Piero Rafanelli
- Corresponding author
- Dipartimento di Astronomia, Universitá di Padova, Vicolo dell'Osservatorio 3, Padova I-35122, Italy
- Other articles by this author:
- De Gruyter OnlineGoogle Scholar
- Dipartimento di Astronomia, Universitá di Padova, Vicolo dell'Osservatorio 3, Padova I-35122, Italy
- Other articles by this author:
- De Gruyter OnlineGoogle Scholar
Published Online: 2017-03-23 | DOI: https://doi.org/10.1515/astro-2017-0351
Open Access
Keywords: instrumentation; telescopes; history of astronomy
About the article
Received: 2011-11-23
Accepted: 2011-11-25
Published Online: 2017-03-23
Published in Print: 2012-06-01
Citation Information: Open Astronomy, Volume 21, Issue 1-2, Pages 1–4, ISSN (Online) 2543-6376, DOI: https://doi.org/10.1515/astro-2017-0351.
© 2017. This work is licensed under the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 License. BY-NC-ND 4.0
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- 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
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