Golden2015 - (other golden conferences)
7-12 September 2015
Palermo, Italy
published May 23, 2017
Palermo, Italy
published May 23, 2017
The purpose of this workshop is to bring together about *80 invited researchers* from world wide to discuss the experimental updated panorama and theories of CVs and Related Objects. The following topics will be discussed:
a) Opening Remarks (the Importance of Multifrequency Observations)
b) Cataclysmic Variables (non-magnetic, intermediate polars, polars)
* Fundamental parameters
* Accretion physics
* Outburst physics
* Magnetic phenomena
* Interconnection among classes
* Long term secular evolution
* The fate of CVs
c) Classical and Recurrent Novae
d) Nova-like Stars
e) Symbiotic stars
f) The Astrophysics of CVs and related Objects with the Ongoing and Future Space-Based and Ground-Based Experiments.
| Sessions |
|---|
| Opening Remarks |
| Cataclysmic Variables |
| Classical Novae, Recurrent Novae and Nova-Like Stars |
| Ongoing Experiments |
| Special Night Session |
| Concluding Remarks |
| Concluding Address |
| Opening Remarks |
|---|
|
The Golden Age of Cataclysmic Variables and Related Objects: The State of Art.
|
|
Stella Physics after Classical-Nova Disaster
|
|
The Impact of AAVSO on Knowledge of CVs and Related Objects
|
|
X-ray Spectroscopy of Accreting White Dwarfs: Prospects for ASTRO-H and Beyond
|
|
Gaia and the use of White Dwarfs as Advanced Physics laboratories
|
|
The impact of SUZAKU on the knowledge of CVs and expectation to ASTRO-H
|
| Cataclysmic Variables |
|
The Propeller White Dwarf Pulsar in AE Aquarii: A Multi-Frequency Emission Laboratory
|
|
Accreting White Dwarfs as Universal Accretion Laboratories
|
|
WD Pulsars and Rotating WD – Theory Vs Observations
|
|
Thermonuclear Burning onto the White Dwarf of CVs
|
|
Binary population models of CVs
|
|
Short Orbital Period Cataclysmic Variables
|
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Connecting Algols to CVs
|
|
Universal accretion on all scales?
|
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Cataclysmic Variables are significant radio emitters
|
|
Low States of Polars: Catalina (CRTS) Light Curves
|
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MHD simulation of column accretion onto a magnetized white dwarf in CVs
|
|
Quasi-periodic oscillations in magnetic Cataclysmic Variables: Results for V834 Cen
|
|
Pre (and post) super soft sources
|
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Observational aspects of magnetic accretion: Doppler tomograghy.
|
|
The transient OT J213806.6+261957 in Pegasus - Possible emitter of gravitational waves
|
|
V1223 Sgr and the long-term activity of the intermediate polars
|
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Assessment the area of accretion curtains from fast aperiodic time variability of Intermediate Polars
|
|
Jets from disc-accreting magnetized stars
|
|
An update on the AM CVn family
|
|
New AM CVn stars and Polars discovered from optical transient surveys
|
|
MASTER-SAAO transient detections: new Cataclysmic Variable discoveries
|
|
The Kepler program for observing interesting CVs
|
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Searching for dead CVs in synoptic surveys
|
|
CVs detected in the XMM-Newton SSC survey of the Galactic plane
|
|
Accretion onto Magnetized Stars: 3D-MHD Simulations
|
|
A large HST program: effective temperatures of cataclysmic variable white dwarfs
|
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GW Librae: A Unique laboratory for pulsations in an accreting white dwarf
|
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SW Sex Stars Then and Now: A Review
|
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Cataclysmic variables in the period gap – the new data
|
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NY Ser: cataclysmic variable in the period gap or The bordeline SU UMa-type dwarf novae
|
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Photometric study of eclipsing dwarf nova GY Cnc above the period gap: active and quiet states
|
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On Candidates of Period Bouncers
|
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QZ Lib - Dwarf Nova and Period Bouncer
|
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Disc Winds Matter! Their Contribution to the Optical Spectra of CVs
|
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Photographic Sky Surveys and Cataclysmic Variables: Recent progress
|
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3D simulations of the interaction between stream from the L1 point and accretion disk in non magnetic CVs
|
|
Accretion Theory: MHD Simulation
|
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The Bounday Layer in compact binaries
|
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Roche tomography of CVs
|
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Spherical and Spatial Distribution of WZ Sagittae Type Dwarf Novae
|
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New cataclysmic binary ASASSN-14fu: orbital and quasi-periodic variability
|
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Research on AM CVn stars: ASASSN-14ei and CR Boo
|
|
Trace elements in WD long term evolution
|
| Classical Novae, Recurrent Novae and Nova-Like Stars |
|
Commemoration of Angelo Cassatella
|
|
Theory of Classical Novae
|
|
Light curve analysis of classical novae: free-free emission vs photospheric emission
|
|
Classical novae in OGLE data
|
|
Isotopic Ratios of 12C-13C and 14N-15N as Clues to Nucleaosynthesis in Novae
|
|
Classical nova V339 Del (Nova Del 2013) - a short review
|
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The nova V1369 Cen – a short review
|
|
Dust grains in the molecular forming Nova V2676 Oph
|
|
Studies of novae in Andromeda Nebula with small telescopes
|
|
When New Becomes Old
|
|
New data on old novae
|
|
Classical novae vs cataclysmic variables
|
|
Multi-mission observations of the old nova GK Per during the 2015 outburst
|
|
Recurrent Novae in the Local Group
|
|
Recurrent Novae: A Masquerade
|
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The recurrent nova T Pyxidis - A review
|
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A remarkable nova in M 31 with a 1-year recurrence time
|
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Multi-frequency Behaviour of Nova-like Systems
|
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Symbiotic stars - a Review
|
|
Supernova type Ia rate enhanced due to new constraints on binary evolution
|
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An alternative channel for type Ia supernovae explosions
|
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Supernova Ia progenitor candidates in the core of planetary nebulae
|
| Ongoing Experiments |
|
The X-ray Astronomy Satellite ASTRO-H
|
|
Study of Cataclysmic Variables with LDS Sky Surveys and ESA Gaia
|
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CVs Astrophysics with LOBSTER and ESA LOFT
|
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SGI (Silicon Graphics International Corp) UV2000: the porting of GFORC system
|
| Special Night Session |
|
What is life for science?
|
|
Who discovered that Hydrogen is the most abundant element in the Cosmos?
|
| Concluding Remarks |
|
Concluding Remarks
|
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Concluding Remarks
|
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Concluding Remarks
|
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The Golden Age of Cataclysmic Variables and Related Objects–III: Concluding Remarks
|
| Concluding Address |
|
Concluding Address
|
