
Accretion is a universal phenomenon that takes place in the vast majority of astrophysical objects. The progress of ground-based and space-borne observational facilities has resulted in the great amount of information on various accreting astrophysical objects, collected within the last decades. The accretion is accompanied by the process of extensive energy release that takes place on the surface of an accreting object and in various gaseous envelopes, accretion disk, jets and other elements of the flow pattern. The results of observations inspired the intensive development of accretion theory, which, in turn, enabled us to study unique properties of accreting objects and physical conditions in the surrounding environment. One of the most interesting outcomes of this intensive study is the fact that accretion processes are, in a sense, self-similar on various spatial scales from planetary systems to galaxies. This fact gives us new opportunities to investigate objects that, by various reasons, are not available for direct study.
Cataclysmic variable stars are unique natural laboratories where one can conduct the detailed observational study of accretion processes and accretion disks. This is the main reason why several participants and a few members of the Organizing Committee of the conference «The Golden Age of Cataclysmic Variables and Related Objects – III» (September 7-12, 2015, Palermo, Italy) have decided to hold a special conference, focused on accretion processes, as a branch of that series.
Main topics:
Young Stellar Objects, protoplanetary discs, exoplanets in binary stars
Accretion on white dwarfs (Cataclysmic variables and related objects)
Accretion on neutron stars (X-ray Binary Systems and related objects)
Accretion on black holes (stellar BH and AGN)
The workshop will include a few 35-minute general review talks to introduce the current problems, and 20-minute talks to discuss new experimental and theoretical results. A series of 15-minute talks will discuss the ongoing and planned ground-based and space-based experiments. There will also be some general talks about the future directions of scientific research on cosmic sources. The papers will pass a peer-review process and the workshop proceedings will be edited by Franco Giovannelli & Lola Sabau-Graziati.
The location of the workshop is the Ambassador Hotel, located in Saint Petersburg, Russian Federation, a venue that will provide a friendly and collaborative atmosphere.
Opening Remarks |
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Accretion Processes in Astrophysics: The State of Art
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The INTEGRAL High Energy Survey: the Accretion Driven Sky
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Simulations of accretion flows in cosmic sources
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The AAVSO as a Resource for Research
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Detecting Gravitation-Wave Memory with LIGO
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Search for Electromagnetic Counterparts of Gravitational Wave Events
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The Impact of the Indian X-ray satellite, AstroSat, on Accretion Processes in Cosmic Sources
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ACCRETION ONTO PLANETS |
Some dynamical similarities among protostellar, AGN, and CV disks
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Protoplanetary Disks – A Review
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Turbulence in Accretion and Protoplanetary Disks
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Observations of Protoplanetary Disks with Subaru
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Accretion on Exoplanets – Formation of Primordial Atmospheres
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The Effect of Coronal Mass Ejection on the Atmosphere of a Hot-Jupiter Exoplanet
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ACCRETION ONTO YOUNG STELLAR OBJECTS AND EVOLUTION |
H2 shocks and mass accretion rate in high mass young stellar objects (HMYSOs)
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Accretion Processes in Massive Star Formation
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Mass Accretion Rates of Pre-Main-Sequence Stars
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Disks Around Young Stars
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Accretion physics in T Tauri stars
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Accretion Processes in CV AM CVn SDSS J090221.35+381941.9
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ACCRETION ONTO WHITE DWARFS, NEUTRON STARS & BLACK HOLES |
Accretion-induced variability links young stellar objects, white dwarfs, and black holes
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Flows and Shocks: Some Recent Developments in Symbiotic Star and Nova Research
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SALT Observations of Accretion Driven Systems
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ACCRETION PROCESSES IN COSMIC SOURCES: The Atmospheres of Accreting White Dwarfs
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Properties of the accretion flow in the Dwarf Novae HL CMa from the properties of the aperiodic variability of its brightness
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Long Term Evolution of Cataclysmic Variables
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Explosive Magnetorotational Instability in Keplerian Disks
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Accretion and Outflows in Accreting White Dwarf Binaries
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Magnetic white dwarfs with debris disks
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Accretion on WD, Observations of Polars
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Features of the Mass Transfer in the Cataclysmic Variable AE Aqr
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Numerical modeling of accretion in EX Hya
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Bow-shocks in disks of young binary systems
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Experimental Indicators of Accretion Processes in Active Galactic Nuclei
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Extracting black-hole rotational energy
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Discovery of Repetitive Optical Variation Patterns from the Accretion Disk During the 2015 Outbursts of the Black Hole X-Ray Binary V404 Cyg
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Be-BH Systems – A Review
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Time lag in transient cosmic accreting sources
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Gamma Ray Emission from Accreting Binaries
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Magnetically driven transient phenomena in accretion driven systems: New breakthroughs with meerKAT and CTA?
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Wind Accretion - Observations Vs Theory
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Accretion Processes on X-ray pulsars
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Extremely-long period X-ray pulsars
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Millisecond pulsar formation in high-mass X-ray binaries
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The OJ 287 black hole binary: witness of the validity of the General Relativity
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Star-jet interactions in AGNs
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Ultraluminous X-ray sources. Optical data.
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KYNREFREV - Implementation of an X-ray Reverberation Model in XSPEC
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Accretion onto Symbiotic Variables
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3D Models of Symbiotic Binaries
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Superhumps in SU UMA Dwarf Novae
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Galactic and extragalactic novae - A Review
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High resolution X-ray spectra of classical and recurrent novae
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Disc-Stream Interaction in Semidetached Binaries
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Introducing Octo-tiger/HPX: Simulating Interacting Binaries with Adaptive Mesh Refinement and the Fast Multipole Method
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Accretion-Outflow Activity in Herbig Ae/Be Stars
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Observing polarimetric variability from CVs to BLAZARS
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Ongoing Experiments |
WSO-UV core program on accretion physics and high energy source
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Geographical Delocalization of FITS Data in MongoDB Environment
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Special Night Session |
Global Warming, Global Warming Pause and the Role of CO2
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Concluding Remarks |
Concluding Remarks
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Concluding Remarks
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Concluding Remarks
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Concluding Remarks
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Concluding Address |
Accretion Processes in Astrophysics: Concluding Address
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