I administrative meetings, deadlines




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Monday, 3 August


11:00 Opening.


11:00 - 12:30 Quasi-periodic oscillations from mHz to kHz. X-ray bursts and superbursts

X-ray bursts and superbursts (I) A. Heger (tbc)

Quasi-periodic oscillations (I) M. Méndez

Energy spectra of LMXB (I) D. Psaltis (tbc)


14:00 - 15:30 X-ray bursts and superbursts. Millisecond X-ray pulsars

Millisecond X-ray pulsars (I) R. Wijnands

X-ray burst ignition and profiles (I) R.L. Cooper

16:00 - 17:30 AXP/SGR and magnetars, very-high energy emission
Discussion and poster summary (30 min)

Magnetars (I) C. Kouveliotou

VHE from neutron stars and their environment (I) F.A. Aharonian

Fast oscillations in SGRs (I) G. Israel (tbc)

Tuesday 4 August



11:00 - 12:30 AXP/SGR and magnetars, isolated neutron stars

Radio pulsars (I) M. McLaughlin

The binary pulsar (I) M. Burgay

Pulsar results from Fermi/GLAST (I) P.S. Ray (tbc)

Wednesday 5 August



11:00 - 12:30 Gravitational waves. Neutron-star equation of state

and strong gravity

Equation of state of neutron stars (I) J.M. Lattimer


14:00 - 15:30 Gravitational waves. Neutron-star equation of state

and strong gravity

Gravitational waves (I) N. Andersson


16:00 -17:30 Future instrumentation for timing. Historical perspective

and future expectations
Free discussion (20 min)

Discussion and poster summary (30 min)

AXTAR mission (I) P.S. Ray (tbc)

ASTROSAT mission (I) D. Bhattacharya (tbc)

HTRS instrument for IXO (I) D. Barret


JD4 Progress in Understanding the Physics of Ap and Related Stars

3 - 5 August 2009


Coordinating Division: IV

SOC chair: Margarida S. Cunha (Portugal).

SOC members: Natalia Drake (Russia), Michael M. Dworetsky (UK), Oleg Kochukhov (Sweden), Friedrich Kupka (Germany), Francis Leblanc (Canada), Lyudmila I. Mashonkina (Russia), Richard Monier (France), Ernst Paunzen (Austria), Nikolai E. Piskunov (Sweden), Hiromoto Shibahashi (Japan), Barry Smalley (UK), Werner W. Weiss (Austria), and Jozef Ziznovsky (Slovakia).

Editors: Margarida S. Cunha, Michael M. Dworetsky & Barry Smalley

Contact: Margarida S. Cunha

URL:


Principal topics

Stellar magnetic fields, atomic diffusion, convection, rotation and pulsations are keys to the general understanding of stars and their evolution. The chemically peculiar (CP) stars provide unique environments in which these physical phenomena interact, both internally and in the atmospheric layers, leaving a multitude of signatures that can be studied using different kinds of observations and techniques. Topics:

  • recent observations and modeling of CP stars as the starting point for a multi-disciplinary exchange of ideas focused on the interpretation of the convolved effects of magnetism, pulsations, convection, rotation, and diffusion, in an evolutionary context

  • current and future ground and space-based observations of CP stars

  • atmospheric modelling and atmospheric mapping in the context of CP stars

  • understanding the CP and related phenomena in the context of stellar evolution.


Preliminary program


I. Pushing the limit of instrument capabilities

Overview on CP stars (I) W.W. Weiss

Current ground-based observations of CP stars (I) S.J. Adelman

Current space-based observations of CP stars (I) J. Matthews

GAIA impact on CP star research (I) D. Shulyak

Discussion ­­– To what degree may complementary techniques

contribute to the understanding of the CP phenomenon?

II. A 3-D look into the atmosphere?

Magnetic fields and chemical inhomogeneities in the upper

layers of hot stars (I) G.A. Wade

Spectral synthesis / atmospheric models (I) L.I. Mashonkina

Pulsations in the atmosphere / inversions (I) T.A. Ryabchikova

Discussion - Atomic data: What do we need as input?

How confidently can we derive Global parameters

of CP stars?

III. CP and related phenomena in the context of stellar evolution

From F- to O-type stars / from pre-main sequence to

WDs: similarities and differences (I) J.D. Landstreet

The origin and evolution of the magnetic field (I) D.L. Moss (tbc)

Stellar evolutionary models: effects of diffusion: recent

work, future plans (I) G.J. Michaud

Stellar evolutionary models: effects of rotation: recent

work, future plans (I) J.-P. Zahn


Discussion - What is the key to the diversity of CP

phenomena? The roles of magnetic fields, rotation,

diffusion, birth environment, and binarity.


IV. Final Discussion - The upcoming challenges of CP star research


JD5 Modelling the Milky Way in the Era of Gaia

6 - 7 August 2009


Coordinating Division: VII

SOC chair: James J. Binney (UK).

SOC members: Luis A.C. Aguilar (Mexico), Herwig B. Dejonghe (Belgium), Kenneth C. Freeman (Australia), Ortwin Gerhard (Germany), Naoteru Gouda (Japan), Amina Helmi (Netherlands), Jacques R.D. Lépine (Brasil), Alice C. Quillen (USA), Annie C.R. Robin (France), and Natalia Y. Sotnikova (Russia).

Editor: James J. Binney

Contact: James J. Binney

URL: < www-thphys.physics.ox.ac.uk/people/JamesBinney/jd5_home.html>


Principal topics

Sophisticated dynamical models will be required to extract science from the large surveys of the Milky Way that will culminate in the Gaia survey (2012-2017). JD5 will review:

  • the kinds of data that are available to constrain such models

  • the various types of dynamical model that could be constructed

  • strategies for fitting models to the data, and

  • the nature of the computational challenge that these processes will entail.

The aims of JD5 are to clarify the work that must be accomplished, and to get the community working collaboratively towards the overall long-term goal.


Preliminary program


Thursday 6 August


I. The challenge

09:00 Star counts, radial velocities, proper motions, metallicities and ages (I) A.C.R. Robin

09:30 Large-scale non-equilibrium structures (I) V. Belokurov

10:00 Non-equilibrium dynamics and radial migration in the disc (I) A.C. Quillen

10:30 coffee

11:00 Star-formation histories, metallicity distributions and

luminosity functions of disk, bulge & halo (I) R.F. Wyse

11:30 Measures of ISM density, absorption, emission at

various frequencies, polarization, Faraday rotation,

dust to gas ratio (I)

12:00 contributed talk

12:15 contributed talk

12:30 lunch

14:00 Gas dynamics: motions driven by bar and spiral

structure (I) F. Combes

14:30 Exploiting horizontal and vertical dynamics of

disc, dynamics of halo structures and satellites (I) A. Helmi

II. Methods

15:00 Introduction to orbit-superposition models.

How do we fit such a model to a catalogue? (I) R.P. van der Marel

15:30 coffee

16:00 contributed talk

16:15 contributed talk

16:30 Torus modelling as an extension of Schwarzschild (I) J.J. Binney

17:00 In what detail can we represent the MW in a

conventional N-body model? (I) V.P. Debattista

Friday 7 August


09:00 To what extent does M2M overcome limitations of

conventional N-body? (I) O. Gerhard

09:30 Projecting models into the observational domain (I) H.B. Dejonghe

10:00 Given the Gaia catalogue, an NIR catalogue (VHS?) and

a dynamical model, how to build a dust model? (I) J.R.D. Lépine

10:30 coffee

11:00 contributed talk

11:15 contributed talk

11:30 How to optimise complex models? Will the computational scale be worryingly large? (I) P. Saha

12:00 - 12:30 Summary (I) K.C. Freeman


JD6 Time and Astronomy

6 - 7 August 2009


Coordinating Division: I

SOC chairs: Pascale Defraigne (Belgium) and Aleksander Brzezinski (Poland).

SOC members: Daniel Gambis (France), Yury P. Ilyasov (Russia), Sergei A. Klioner (Germany), Michael Kramer (UK), Richard N. Manchester (Australia), Demetrios N. Matsakis (USA), Rendong Nan (China Nanjing), and Gérard Petit (France).

Editors: Pascale Defraigne & Aleksander Brzezinski

Contact: Pascale Defraigne


URL:


Principal topics

  • aspects of time, its use for astronomy, and the contributions from astronomy

  • Earth rotation and time: an overview of UT1 determination as well as UT1 modeling and prediction

  • atomic time scales: the present realizations and performance of atomic time scales and time transfer techniques.

  • pulsar timing and its applications: recent developments in precision

  • pulsar timing and its application to time scales, planetary ephemerides, detection of gravitational waves and tests of gravitational theories.


Preliminary program


I. Earth rotation and time

UT1/LOD realization and accuracy

Geophysical impact on UT1

Short- and long-term variations of UT1

Use of UT1 for astro-geodetic studies

UT1 prediction


II. Atomic time scales

Stability of TAI, TT(BIPM)

Impact of new frequency standards on SI time scales

GNSS time scales

Time transfer

Recent developments with leap seconds


III. Pulsar timing and its applications

Techniques of precision pulsar timing

Pulsar time scales

Pulsar tests of gravitational theories

Pulsar timing arrays and detection of gravitational waves

Improving solar-system ephemeredes

Pulsar timing noise


JD7 Astrophysical Outflows and Associated Accretion Phenomena

6 - 7 August 2009


Coordinating Division: VI

SOC chairs: Elisabete M. de Gouveia Dal Pino (Brasil) and Alejandro C. Raga (Mexico).

SOC members: Mark Birkinshaw (UK), Sylvie Cabrit (France), Max Camenzind (Germany), Adriano H. Cerqueira (Brasil), Atillio Ferrari (Italy), I. Felix Mirabel (Chile), R. Naryan (USA), Thomas P. Ray (Ireland), F. Felipe Rodriguez (Mexico), K. Shibata (Japan), James M. Stone (USA), and Thaisa Storchi-Bergmann (Brasil).

Editors: Elisabete M. de Gouveia Dal Pino & Alejandro Raga

Contact: Elisabete M. de Gouveia Dal Pino

URL:


Principal topics

Highly collimated supersonic jets and outflows are very frequent in several astrophysical environments. Despite their different physical scales, all these outflow classes have strong morphological similarities.

  • what physics do they share?

  • can we find a universal mechanism of acceleration and collimation that operates in all classes?

  • the origin of the astrophysical jets and their effects on the astrophysical environments

  • understanding the driving mechanisms of jets from proto-stars (including their possible crucial link with star and planet formation) to microquasars and AGNs

  • the basic physics of the accretion-jet process in magnetized disks, including the transport of angular momentum and the development of reconnection and turbulent dynamo

  • cooling/heating processes, instabilities, shock structures and particle acceleration mechanisms in the jets

  • the impact of the jets on energy balance and turbulence feeding in the astrophysical environments

  • the potential association of jet-accretion phenomena with GRBs and UHECRs.


Preliminary program


Thursday 6 August      


09:00 Welcoming address E.M. de Gouveia Dal Pino & A.C. Raga

I. Jet/Accretion Disk systems: basic physics

09:05 Numerical simulations of MHD accretion disks (I) J.F. Hawley

Jet-accretion disk physics: from transport to dynamo

processes (I) A.R. King

Accretion disks theory (I) R. Narayan

panel / poster discussion

10:30 coffee break /poster viewing


II. Jet observations in all scales

11:00 YSO jets optical observations (I) B. Reipurth

YSO jets rotation and magnetic field observations (I) T.P. Ray

QPO-Jet relation in X-ray binaries and AGNs (I) T. Belloni

Extragalactic jet observations from radio to X-ray /

acceleration (I) M. Birkinshaw

panel / poster discussion

12:30 lunch


III. Jet launching

14:00 Numerical MHD simulations of astrophysical jets (I) K. Shibata

Magnetic Reconnection in accretion

disk/corona and jet launching (I) E.M. de Gouveia Dal Pino

AGN accretion disk observations (I) T. Storchi-Bergmann

Are jets rotating at the launching? (I) N. Soker

panel / poster discussion


15:30 coffee break / poster viewing


IV. Jet propagation and interaction with environment in all scales

16:00 Is there an UHECRs-AGN connection? (I) P.L. Biermann (tbc)

Extragalactic jets simulations (I) A. Ferrari

YSO jet simulations (I) A.C. Raga

panel /poster discussion


Friday  7 August


V. Jets from YSOs

09:00 YSO radio and milimmetric observations (I) L.F. Rodriguez

Star formation-jet connection (I) F.H. Shu

Jet-accretion connection in YSOs (I) S. Cabrit

panel / poster discussion

10:30 coffee break / poster viewing


VI. Relativistic Jets: GRBs, BHs, new generation instruments

11:00 Jets in GRBs (I) P. Meszaros

Theory of relativistic jets (I) M. Camenzind

Accretion/jet connection in black holes – observations (I) I.F. Mirabel

ALMA and LOFAR in the context of accretion disks (I) A. Dutrey


Summary and concluding remarks A.C. Raga & E.M. de Gouveia Dal Pino


JD8 Hot Interstellar Matter in Elliptical Galaxies

6 - 7 August 2009


Coordinating Division: VIII

SOC chairs: Dong-Woo Kim (USA) and Silvia Pellegrini (Italy).

SOC members: Françoise Combes (France), Sofia A. Cora (Argentina), Giuseppina Fabbiano (USA), Alexis Finoguenov (Germany), Brad K. Gibson (UK), Nimisha G. Kantharia (India), Chiaki Kobayashi (Japan), Cláudia L. Mendes de Oliveira (Brasil), Elaine M. Sadler (Australia), Craig L. Sarazin (USA), Thomas S. Statler (USA), and Ginevra Trinchieri (Italy).

Editors: Dong-Woo Kim & Silvia Pellegrini

Contact: Dong-Woo Kim

URL:
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